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\begin{document}

\begin{titlepage}
\vspace*{1.4cm}

\begin{center}
{\huge
{\bf A General Catalogue of

Herbig-Haro Objects}
}
\vspace*{0.6cm}

{\Large\bf 2. Edition}

\vspace*{2.5cm}

{\Large{\bf Bo Reipurth}}
\vspace*{0.4cm}

{\large

Center for Astrophysics and Space Astronomy \\
University of Colorado \\
Campus Box 389, Boulder, CO 80309 \\
USA

reipurth@casa.colorado.edu



}

\vspace{7cm}

{\Large{\bf Electronic Version 1999}}

\vspace{0.5cm}

http://casa.colorado.edu/hhcat

\end{center}
\end{titlepage}

\newpage

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\vspace*{2cm}

\begin{center}
{\Large {\bf Abstract}}
\end{center}

A catalogue of all known Herbig-Haro objects is presented. For each
object is given its HH number, previous designations if any, a
position, the most probable energy source, and the region and
distance. Additionally, extensive notes give a brief description of each
object with detailed references to the literature. The catalogue will
be updated as developments in the field require.

\vspace*{6cm}

\begin{center}

\fboxrule0.02cm
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\fbox{\rule[-0.9cm]{0.0cm}{1.8cm}{\parbox{15cm} 
{
This catalogue will not be published in any journal. It is 
only available through the WWW at http://casa.colorado.edu/hhcat

\vspace*{0.5cm}

Reference to this catalogue should be done as follows: 

\vspace{0.2cm}

Reipurth, B.: 1999, {\em A general catalogue of Herbig-Haro objects},
2.~edition,\\
 http://casa.colorado.edu/hhcat

}}}

\end{center}

\newpage

\begin{center}
{\Large {\bf Introduction}}

\end{center}

Two catalogues of Herbig-Haro objects have previously been published.
George Herbig's {\em A draft catalog of Herbig-Haro objects} from
1974 gave positions, finding charts and a brief description of all 43
objects known up to that time. This was followed by {\em A working
catalogue of Herbig-Haro objects} by von Hippel, Burnell, Williams
(1988), which gave positions, proper motions, radial velocities and
spectral information for 89 HH objects or groups of HH knots, although
more HH objects were known at the time. Since then the increasingly
common use of large-field CCD detectors with interference filters have
caused an almost explosive development in the discovery rate of HH
objects, which now number more than 400 objects.

In the days when discoveries of HH objects were rare and only few
people worked in the field it was possible to assign consecutive HH
numbers to the objects as they became known. This has long since
become impossible, and lacking some sort of coordinating facility,
newly discovered HH objects have been given a great variety of names
(e.g. S140/HH3, GGD 34, N2264~HH 14-4, RNO 40E, WSB 47, Re 4 head,
GN20.18.3/HH, Th~28, HHG33.3+0.2).

Some years ago I was approached by Dr. M.-C. Lortet of the IAU
Nomenclature Committee, who asked me if something could be done to
bring order to this wild growing subject. After some hesitation I
embarked upon a survey of the entire literature on Herbig-Haro flows
with the aim to produce a complete catalogue of all known HH objects,
and the result was the first edition of {\em A General Catalogue of
Herbig-Haro Objects}, published electronically in 1994.  The present
second edition has been greatly expanded over the intervening 5 years.
The philosophy of this catalogue is closer to that of Herbig's 1974
catalogue than to that of the von Hippel, Burnell, Williams 1988
catalogue. The present catalogue contains three parts.  First, a table
listing for each object an HH number, any previous designations, a
position, identification of a suspected driving source, the name of
the general region of the object, and a distance estimate.  Second, a
note section where each object is briefly described and extensive references, 
as complete as possible, are given to the literature. Third,
a section with references, where also the title is listed, to help
give a first idea about the content of a paper.  The catalogue is thus
less a source of information, and more a tool to find information.

All known HH objects accepted as such now have an HH number, in
continuation of the already existing HH numbers assigned by Herbig and
others. In most cases this is a great improvement over previous
designations. In a few cases well known and beloved names have been
sacrificed, with regret, for the sake of the larger vision of having
once and for all a single nomenclature system that gives a complete
description of an increasingly important class of astrophysical
objects. When an object had to be renamed, a special effort was made
to find a number that, whenever possible, was somehow related to the
previous name. Thus RNO 40 and 43 are now HH 240 and 243, Th~28 is HH
228, M16-HH1 is HH 216, the M42 objects HH 1-10 are HH 201 - 210,
GGD34 is HH~234, etc. Hopefully any transition difficulties will be
shortlived.


\newpage

\begin{center}

{\bf What is an HH object (and what is not)?}

\end{center}


In the course of this work, the question has inevitably arisen a
number of times whether a certain object should or should not be
included in the catalogue. While it is impossible to make very strict
rules for what to include, at least a set of guidelines have been set
up. HH objects are small-scale shock regions intimately associated
with star forming regions. They generally have characteristic spectra
which set them apart from photo-ionized regions. The best way to
unequivocally identify a nebulous object in a star forming region as
an HH object is to take a spectrum. Increasingly, however, a simpler
technique is used, namely to take CCD images through a [SII]
interference filter and through either a similar slightly blue- or
red-shifted filter that avoids the [SII] lines or through a red
broadband filter around 0.9 or 1.0 $\mu$m that transmits only few and
weak HH lines. If the object observed appears strongly in the [SII]
filter, but not in the other filter then it is virtually certain that
the object is an HH object.  However, this method becomes questionable
if applied in regions away from molecular clouds and known star
formation activity.

Another technique, pioneered by Solf, is to place a long slit on a
young star at a variety of position angles. Very short HH flows, that
would be difficult to see in a direct image where the brightness of
the star could swamp it, will appear clearly after elimination of the
stellar continuum. I have used the guideline that such flows that
extend more than an arcsecond from a star, and which could thus in
principle be studied morphologically using proper coronagraphic
techniques, are included in the catalogue. Stars with HH emission
lines but no appreciable extent have not been included.

With the advent of infrared imaging detectors, many HH objects have
been found to emit significantly in H$_2$ and [FeII], with roughly
similar morphologies at optical and infrared wavelengths. A number of
molecular hydrogen objects have been detected in embedded molecular
outflows with no optical counterparts. While it seems probable that
these objects differ from ordinary HH objects only in the amount of
extinction along the line-of-sight, much work on the infrared
properties of HH flows remains to be done before it can be justified
to expand the definition of HH objects to include all objects only
detected in the infrared. However, for the first edition of this
catalogue, this rule was relaxed for a few objects with additional
strong morphological support for classification as an HH flow. Thus,
HH~121 and HH~211, which are well collimated bipolar flows, located in
regions of star formation and up to now only detected at infrared
wavelengths, were included (two more objects, HH~212 and HH~288, which
were first discovered as infrared objects, have subsequently been
found to have some optical bona fide HH components). In hindsight, it
must be recognized that it was not a good idea to make such
exceptions, and consequently no further purely infrared emitting
objects have been included in this HH catalogue.

In recent years an increasing number of shocked regions have been
found in association with evolved stars. Kinematically and
morphologically these objects do not appear to differ much from
Herbig-Haro objects, but spectroscopically they are rather different
because the shocks occur in highly processed material. From the point
of view of hydrodynamics and shock physics these objects are
undoubtedly as interesting as HH flows and supernova remnants and
other supersonic flows. However, the most important aspect of the
Herbig-Haro phenomenon is arguably the unique insights which it has
provided into the processes that lead to the formation of stars. For
this reason it was felt that HH flows should remain strictly as a star
formation phenomenon, as it was originally defined by Herbig and
Haro. Thus, this catalogue does not contain any objects which arise
from evolved stars.

%\newpage

\begin{center}

{\bf Electronic publishing}

\end{center}

Electronic publishing has two major advantages. Firstly, it allows
instantaneous and worldwide distribution without the long delays
inherent in normal publishing.  Secondly, it allows easy up-dating as
often as required. It was originally foreseen that new versions of
this catalogue would be made available of the order of once a year.
However, in practice it has turned out to be so time consuming to keep
track of the greatly expanding literature on HH objects, that five
years have passed between the first and second version of the
catalogue. I will continue to update the catalogue as the need arises
and time permits.  New versions will be announced in the {\em Star
Formation Newsletter}.

The literature listed in this second edition is complete for papers
published before 1 March 1999.

A limitation of the present catalogue is the absence of images of the
various HH objects. However, work is rapidly progressing on a
web-based version which includes images of each HH object. The next
version of this catalogue will be an illustrated and fully linked web
version.

\begin{center}

{\bf A cooperative effort}

\end{center}

New bona fide Herbig-Haro objects will, as they appear in the
literature, continue to be included in the catalogue. But if you have
found a new HH object, you may consider to contact me when you are in
the final stages of writing your paper, to find out what is the next
available HH number. Unless waived, all such information will be
treated as confidential and will not appear in new versions of the
catalogue until your paper is accepted. New HH objects are
continuously having numbers reserved this way, so {\em please do not
simply take the next apparently free HH number as this could cause
grave confusion}.  With a collaborative effort among the workers in
the Herbig-Haro community it will be possible to establish this
catalogue and its future expanded editions as a tool that will make
our work easier.  Your cooperation in this matter is highly
appreciated.

While a major effort has been invested in making the references to
work on individual objects as complete as possible, it is inevitable
that some important references could be missing. Certainly not all
papers mentioning a given object should be listed, and an estimate of
relevance has been applied to all papers. For a little known object
even a single poor observation can be helpful, but it could be
irrelevant for very well studied regions like L1551. So no universal
rule of inclusion can be made. If you feel that a useful reference is
missing, please send an e-mail to me at {\em reipurth@casa.colorado.edu}.

\begin{center}

{\bf Accuracy of positions}

\end{center}

The positions listed in the catalogue are taken from the literature
and are as such very heterogeneous. An effort has been made to take
the best available positions, but in some cases the positions are
rather approximate. The equinox is 1950 and proper motions have not
been considered.  The goal has been to give positions that will allow
an observer to point a telescope and take a CCD image and be sure that
the object or an important part of it is in the field. For more
details on positions, the reader must consult the references listed.


\begin{center}

{\bf Acknowledgements}

\end{center}

I am grateful to the following persons, who have generously given of
their time to comment on this catalogue prior to publication, or have
supplied information: Vicky Alten, Colin Aspin, John Bally, Karl-Heinz
B\"ohm, Jose Cernicharo, Chris Davis, David Devine, Jochen
Eisl\"offel, Mercedes G\'omez, George Herbig, Stacy Mader, Tigran
Magakyan, Mark McCaughrean, Reinhard Mundt, Bob O'Dell, Alex Raga, Tom
Ray, Luis Felipe Rodr\'\i guez, Richard Schwartz, Karl Stapelfeldt,
Karen Strom, Jos\'e Torrelles, Bruce Wilking, Jan Wouterloot, Jun Yan,
Ji Yang, Ka Chun Yu, Joao Lin Yun, Hans Zinnecker.


\vspace*{1cm}

Boulder, Colorado 1 May 1999~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~Bo Reipurth







\newpage

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\begin{center}

{\Large{\bf Catalogue of Herbig-Haro Objects}}

\vspace*{0.5cm}

\begin{tabular}{|r|p{2.9cm}|r|r|p{2.7cm}|p{2cm}|r|}\hline
\multicolumn{1}{|c|}{HH} &
\multicolumn{1}{c|}{Other} &
\multicolumn{1}{c|}{$\alpha_{1950}$} &
\multicolumn{1}{c|}{$\delta_{1950}$} &
\multicolumn{1}{c|}{Suspected} &
\multicolumn{1}{c|}{Region} &
\multicolumn{1}{c|}{Dist} \\
 & \multicolumn{1}{c|}{designation} & & & \multicolumn{1}{c|}{source} & &
\multicolumn{1}{c|}{$[$pc$]$}  \\ \hline
  &&&&&& \\

161 & LkH$\alpha$ 198B/HH &   0 08 48.9 & +58 32 45 & LkH$\alpha$ 198-B & Cassiopeia  & 950  \\
164 & LkH$\alpha$ 198 jet &   0 08 47.5 & +58 32 48 & LkH$\alpha$ 198 & Cassiopeia & 950 \\
162 & V376 Cas/HH & 0 08 49.8 & +58 33 27 & V376 Cas   & Cassiopeia & 950  \\ 
461 &         &  0 08 52.0 &  +58 31 35 & LkH$\alpha$ 198-B & Cassiopeia & 950 \\
288 &         &  0 34 18.6 &  +63 47 45 & IRAS00342+6347 & Cassiopeia & 2000 \\
163 & AFGL4029 jet & 2 57 36.0 & +60 17 22 & AFGL 4029  & IC1848A  & 2200  \\
280 &          &  3 20 40.5 &  +30 07 22 &            & Perseus  & 300 \\
267 &          &  3 20 58.3 &  +30 49 53 &            & L1448    & 300 \\
268 &          &  3 21 17.6 &  +30 37 36 &            & L1448    & 300 \\
193 &          &  3 21 48.1 &  +30 44 22 &            & L1448    & 300 \\
194 &          &  3 21 54.1 &  +30 37 09 &            & L1448    & 300 \\
196 &          &  3 22 08.9 &  +30 38 46 &            & L1448    & 300 \\
195 &          &  3 22 10.4 &  +30 36 28 &            & L1448    & 300 \\
197 &          &  3 22 32.3 &  +30 34 32 &            & L1448    & 300 \\
277 &          &  3 23 00.1 &  +30 28 51 &            & L1448    & 300 \\
278 &          &  3 23 55.1 &  +30 15 32 &            & Perseus  & 300 \\
317 &          &  3 24 07.3 &  +30 01 34 &            & L1455    & 300 \\
279 &          &  3 24 14.5 &  +30 06 51 &            & Perseus  & 300 \\
423 &          &  3 24 30.9 &  +30 05 30 &            & L1455    & 300 \\
318 &          &  3 24 40.5 &  +30 03 54 &            & L1455    & 300 \\
422 &          &  3 24 43.9 &  +30 01 15 &            & L1455    & 300 \\
338 &          &  3 25 07.3 &  +31 09 22 &            & NGC 1333 & 220 \\
351 &          &  3 25 13.0 &  +30 40 09 &            & NGC 1333 & 220 \\
339 &          &  3 25 25.5 &  +31 04 25 &            & NGC 1333 & 220 \\
340 &          &  3 25 39.7 &  +30 55 19 &            & NGC 1333 & 220 \\
 13 &          &  3 25 42.1 &  +30 56 47 &            & NGC 1333 & 220 \\
 14 &          &  3 25 44.4 &  +30 50 56 &            & NGC 1333 & 220  \\
341 &          &  3 25 44.8 &  +30 59 16 &            & NGC 1333 & 220 \\
334 &          &  3 25 46.0 &  +31 12 19 &            & NGC 1333 & 220 \\
342 &          &  3 25 46.5 &  +31 00 29 &            & NGC 1333 & 220 \\
343 &          &  3 25 49.1 &  +30 55 02 &            & NGC 1333 & 220 \\
426 &          &  3 25 49.3 &  +30 42 07 &            & NGC 1333 & 220 \\
350 &          &  3 25 49.6 &  +30 54 22 &            & NGC 1333 & 220 \\
 12 &          &  3 25 52.1 &  +31 09 51 & SVS~12     & NGC 1333 & 220  \\
 15 &          &  3 25 53.5 &  +30 57 43 &            & NGC 1333 & 220  \\
344 &          &  3 25 56.2 &  +31 02 57 &            & NGC 1333 & 220 \\
 11 &          &  3 25 59.0 &  +31 05 35 & SVS~13     & NGC 1333 & 220  \\
 10 &          &  3 25 59.8 &  +31 05 28 & SVS~13     & NGC 1333 & 220  \\
  8 &          &  3 26 00.7 &  +31 05 19 & SVS~13     & NGC 1333 & 220  \\
  9 &          &  3 26 00.9 &  +31 05 35 & SVS~13     & NGC 1333 & 220  \\
  7 &          &  3 26 02.5 &  +31 05 10 & SVS~13     & NGC 1333 & 220  \\
 16 &          &  3 26 02.8 &  +30 58 52 &            & NGC 1333 & 220  \\
333 &          &  3 26 06.1 &  +31 15 51 &            & NGC 1333 & 220  \\
345 &          &  3 26 09.6 &  +31 03 08 &            & NGC 1333 & 220 \\
  6 &          &  3 26 07.0 &  +31 08 23 &            & NGC 1333 & 220  \\
347 &          &  3 26 10.2 &  +31 05 04 &            & NGC 1333 & 220 \\
335 &          &  3 26 12.0 &  +31 12 45 &            & NGC 1333 & 220  \\
352 &          &  3 26 13.1 &  +30 49 46 &            & NGC 1333 & 220 \\
  &&&&&& \\ \hline \end{tabular}

\begin{tabular}{|r|p{2.9cm}|r|r|p{2.7cm}|p{2cm}|r|}\hline
\multicolumn{1}{|c|}{HH} &
\multicolumn{1}{c|}{Other} &
\multicolumn{1}{c|}{$\alpha_{1950}$} &
\multicolumn{1}{c|}{$\delta_{1950}$} &
\multicolumn{1}{c|}{Suspected} &
\multicolumn{1}{c|}{Region} &
\multicolumn{1}{c|}{Dist} \\
 & \multicolumn{1}{c|}{designation} & & & \multicolumn{1}{c|}{source} & &
\multicolumn{1}{c|}{$[$pc$]$}  \\ \hline
  &&&&&& \\


 17 &          &  3 26 14.7 &  +31 08 17 &            & NGC 1333 & 220  \\
  5 &          &  3 26 14.8 &  +31 02 34 &            & NGC 1333 & 220  \\
346 &          &  3 26 16.0 &  +31 05 10 &            & NGC 1333 & 220 \\
  4 &          &  3 26 18.6 &  +31 09 41 &            & NGC 1333 & 220  \\
348 &          &  3 26 19.9 &  +31 03 17 &            & NGC 1333 & 220 \\
 18 &          &  3 26 21.0 &  +30 57 21 &            & NGC 1333 & 220  \\
336 &          &  3 26 30.1 &  +31 09 08 &            & NGC 1333 & 220 \\
349 &          &  3 26 30.7 &  +31 03 16 &            & NGC 1333 & 220 \\
353 &          &  3 26 32.2 &  +31 19 56 &            & NGC 1333 & 220 \\
368 &          &  3 27 19.2 &  +30 20 43 &            & Barnard 1 & 220 \\
369 &          &  3 27 22.3 &  +30 18 11 &            & Barnard 1 & 220 \\
370 &          &  3 27 28.3 &  +30 17 31 &            & Barnard 1 & 220 \\
427 &          &  3 27 33.1 &  +30 11 43 &            & Barnard 1 & 220 \\
371 &          &  3 27 41.2 &  +30 20 45 &            & Barnard 1 & 220 \\
372 &          &  3 27 41.2 &  +30 19 13 &            & Barnard 1 & 220 \\
428 &          &  3 27 42.4 &  +30 27 51 &            & Barnard 1 & 220 \\
429 &          &  3 28 42.4 &  +30 59 50 &            & Barnard 1 & 220 \\
430 &          &  3 29 21.7 &  +31 14 32 &            & Barnard 1 & 220 \\
356 &          &  3 29 59.8 &  +31 16 39 &            & Barnard 1 & 220 \\
431 &          &  3 30 09.2 &  +30 59 04 & IRAS03301+3057 & Barnard 1 & 220 \\
432 &          &  3 30 27.5 &  +30 59 41 &            & Barnard 1 & 220 \\
433 &          &  3 30 43.7 &  +30 54 55 & IRAS03304+3100 & Barnard 1 & 220 \\
211 &          &  3 40 48.2 &  +31 51 28 &            & IC 348   & 300 \\
366 &          &  3 43 49.7 &  +32 36 05 & B5 IRS1    & B5       & 350 \\
367 &          &  3 43 57.9 &  +32 33 05 & B5 IRS3    & B5       & 350 \\
462 &          &  3 50 46.8 &  +38 01 46 & IRAS03507+3801 & Perseus & 350 \\
362 &          &  4 01 20.5 &  +26 12 31 &            & L1489 & 140\\
361 &          &  4 01 32.4 &  +26 13 35 &            & L1489  & 140\\
360 &          &  4 01 40.5 &  +26 10 51 &            & L1489   & 140\\
463 & PP13S jet & 4 07 20.9 &  +38 00 03 & PP13S      & L1473   & 350 \\
464 &           & 4 07 22.4 &  +37 59 52 & PP13N      & L1473   & 350 \\
465 &           & 4 07 22.4 &  +38 00 47 & PP13N      & L1473   & 350 \\
220 & CW Tau jet & 4 11 11.3 & +28 03 27 & CW Tau     & Taurus   & 140 \\
156 & CoKu Tau-1 jet & 4 15 45.4 & +28 13 14 & CoKu Tau-1 & Taurus & 140  \\
390 &          &  4 16 36.1 &  +27 08 42 & IRAS04166+2706 & Taurus & 140 \\
391 &          &  4 16 51.7 &  +27 02 16 & IRAS04169+2702 & Taurus & 140 \\
392 &          &  4 17 49.8 &  +26 52 46 &                & Taurus & 140 \\ 
355 &          &  4 18 48.1 &  +19 43 40 & T Tauri    & Taurus   & 140 \\
157 & Haro 6-5B jet  & 4 18 56.4 & +26 50 36 & Haro 6-5B  & Taurus & 140  \\
155 & HH 1555  &  4 19 01.9 &  +19 25 05 & T Tauri    & Taurus   & 140  \\
276 &          &  4 19 02.8 &  +26 50 25 &            & Taurus   & 140 \\
255 & Burnham's Nebula & 4 19 04.2 & +19 24 55 & T Tau-S & Taurus & 140 \\
300 &          &  4 22 21.7 & +24 16 32  & IRAS04329+2436 & B18   & 140 \\
159 & DG Tau B jet & 4 23 58.4 & +25 59 00 & DG Tau B & Taurus   & 140  \\
158 & DG Tau jet & 4 24 01.0 & +25 59 35 & DG Tau     & Taurus   & 140  \\
410 &          &  4 25 11.6 &  +24 12 25 & Haro 6-10   & Taurus & 140 \\
 31 &          &  4 25 14.4 &  +26 11 04 & IRAS04248+2612 & B218     & 140  \\
184 & Haro 6-10/HH & 4 26 21.9 & +24 26 29 & Haro 6-10 & Taurus & 140 \\
414 &          &  4 26 28.4 &  +24 33 22 & IRAS04264+2433 & Taurus & 140 \\
412 &          &  4 26 46.1 &  +24 30 40 & Haro 6-10   & Taurus & 140 \\
413 &          &  4 26 51.1 &  +24 31 42 & IRAS04264+2433 & Taurus & 140 \\
  &&&&&& \\ \hline \end{tabular}

\begin{tabular}{|r|p{2.9cm}|r|r|p{2.7cm}|p{2cm}|r|}\hline
\multicolumn{1}{|c|}{HH} &
\multicolumn{1}{c|}{Other} &
\multicolumn{1}{c|}{$\alpha_{1950}$} &
\multicolumn{1}{c|}{$\delta_{1950}$} &
\multicolumn{1}{c|}{Suspected} &
\multicolumn{1}{c|}{Region} &
\multicolumn{1}{c|}{Dist} \\
 & \multicolumn{1}{c|}{designation} & & & \multicolumn{1}{c|}{source} & &
\multicolumn{1}{c|}{$[$pc$]$}  \\ \hline
  &&&&&& \\






411 &          &  4 27 14.9 &  +24 36 14 & Haro 6-10   & Taurus & 140 \\
393 &          &  4 27 48.6 &  +24 34 59 &             & Taurus & 140 \\
256 & GH 1     &  4 27 59.5 &  +17 52 41 & L1551 IRS 5 & L1551  & 140 \\
257 & GNG 17   &  4 28 07.0 &  +17 54 17 & L1551 IRS 5 & L1551  & 140 \\
258 & GH 2-8   &  4 28 11.0 &  +17 57 07 & L1551 IRS 5 & L1551  & 140 \\
 28 &          &  4 28 13.2 &  +17 56 58 & L1551 IRS 5 & L1551  & 140 \\
259 & SH 229 group & 4 28 20.3 & +17 57 38 & L1551 IRS 5 & L1551 & 140 \\
265 & GNG 25   &  4 28 21.0 &  +18 05 35 &            & L1551    & 140 \\
264 & GNG 4    &  4 28 24.6 &  +17 59 52 &            & L1551    & 140 \\
102 & S239     &  4 28 25.3 &  +18 00 57 &            & L1551    & 140  \\
263 & SH 214, GNG 3 & 4 28 29.5 & +18 01 24 &         & L1551    & 140 \\
260 & GNG 1    &  4 28 33.1 &  +18 00 31 & L1551 IRS 5 & L1551   & 140 \\
 29 &          &  4 28 33.2 &  +18 00 00 & L1551 IRS 5 & L1551  & 140 \\
261 & SH 219/220 & 4 28 36.1 & +18 00 30 & L1551 IRS 5 & L1551  & 140 \\
154 & L1551 IRS5 jet & 4 28 39.9 & +18 01 39 & L1551 IRS 5 & L1551 & 140  \\
 30 &          &  4 28 43.6 &  +18 06 03 & HH 30~IRS   & L1551    & 140  \\
150 & HL Tau jet & 4 28 44.5 & +18 07 36 & HL Tau     & L1551    & 140  \\
153 & HL Tau H$\alpha$ jet & 4 28 45.4 & +18 07 16 & & L1551    & 140  \\
151 & HL Tau VLA1 jet & 4 28 45.6 & +18 07 45 & HL Tau VLA1 & L1551 & 140  \\
152 & XZ Tau jet & 4 28 46.1 & +18 07 35 & XZ Tau    & L1551    & 140  \\
454 &          &  4 28 48.8  & +18 01 57 & L1551-NE  & L1551    & 140 \\
266 & GNG 24   &  4 28 58.2  & +18 10 28 &           & L1551    & 140 \\
262 & GH 9/10  &  4 29 07.1  & +18 05 03 & L1551 IRS 5 & L1551  & 140 \\
319 & Haro 6-19 & 4 29 39.4  & +24 15 27 &           & Taurus   & 140 \\
286 &          &  4 29 47.6  & +18 10 18 &           & L1551    & 140 \\
394 &          &  4 30 12.5  & +22 48 53 & IRAS04302+2247 & Taurus & 140 \\ 
467 &          &  4 30 31.2  & +24 14 12 &           & B18      & 140 \\
466 &          &  4 30 33.7  & +24 15 17 & GK Tau    & B18      & 140 \\
468 &          &  4 30 35.9  & +24 15 28 &           & B18      & 140 \\
123 &          &  4 32 31.7 &$-$14 19 17 & L1642-2A   & L1642    & 125  \\  
378 &          &  4 32 39.6 &  +54 32 07 & IRAS04327+5432 & Camelopardalis & ?  \\
230 & DO Tau jet & 4 35 24.2 & +26 04 55 & DO Tau     & Taurus   & 140 \\
233 &          &  4 35 30.9 & +26 04 45  & HV Tau     & Taurus   & 140 \\
192 &          &  4 36 43.4 &  +25 57 37 &            & L1527    & 140 \\
395 &          &  4 37 04.8 &  +25 40 56 & IRAS04369+2539 & Taurus & 140 \\ 
408 &          &  4 38 34.7 &  +25 50 44 & Haro 6-33  & Taurus   & 140 \\
231 & DP Tau jet & 4 39 34.3 & +25 10 00 & DP Tau     & Taurus   & 140 \\
386 & UY Aur jet & 4 48 35.7 & +30 42 14 & UY Aur     & Auriga   & 140 \\
229 & RW Aur jet & 5 04 37.7 & +30 20 14 & RW Aur     & Auriga   & 140 \\
114 &          &  5 15 00.7 &  +07 12 39 & IRAS05155+0707 & L1589 & 470  \\
328 &          &  5 15 13.4 &  +07 12 47 &            & L1589 & 470 \\
329 &          &  5 15 58.6 &  +07 05 12 &            & L1589 & 470 \\
115 &          &  5 16 03.7 &  +07 02 21 & IRAS05155+0707 & L1589 & 470  \\
240 & RNO 40   &  5 17 13.8 &$-$05 54 45 & IRAS05173$-$0555 & Orion & 470 \\
241 & RNO 40-E &  5 17 31.3 &$-$05 55 23 & IRAS05173$-$0555 & Orion & 470 \\
190 &          &  5 27 27.5 &  +33 45 38 &                & AFGL 5142 & 470 \\
 58 &          &  5 28 22.7 &$-$04 11 44 &            & Orion    & 470  \\
176 &          &  5 28 38.3 &  +12 08 43 & HK Ori         & $\lambda$ Ori & 470 \\
179 &          &  5 29 14.5 &  +12 33 16 & IRAS05295+1247 & $\lambda$ Ori & 470 \\
244 &          &  5 29 24.0 &  +12 43 55 & IRAS05295+1247 & $\lambda$ Ori & 470 \\
  &&&&&& \\ \hline \end{tabular}

\begin{tabular}{|r|p{2.9cm}|r|r|p{2.7cm}|p{2cm}|r|}\hline
\multicolumn{1}{|c|}{HH} &
\multicolumn{1}{c|}{Other} &
\multicolumn{1}{c|}{$\alpha_{1950}$} &
\multicolumn{1}{c|}{$\delta_{1950}$} &
\multicolumn{1}{c|}{Suspected} &
\multicolumn{1}{c|}{Region} &
\multicolumn{1}{c|}{Dist} \\
 & \multicolumn{1}{c|}{designation} & & & \multicolumn{1}{c|}{source} & &
\multicolumn{1}{c|}{$[$pc$]$}  \\ \hline
  &&&&&& \\

243 & RNO 43   &  5 29 39.0 &  +12 51 12 & IRAS05295+1247 & $\lambda$ Ori & 470 \\
245 & RNO 43-N &  5 29 44.3 &  +12 56 05 & IRAS05295+1247 & $\lambda$ Ori & 470 \\
 59 &          &  5 29 52.0 &$-$06 31 09 &            & Orion    & 470  \\
 60 &          &  5 30 11.4 &$-$06 28 50 &            & Orion    & 470  \\
 83 & Re 17    &  5 31 05.4 &$-$06 31 39 & HH 83 IRS  & L1641    & 470  \\
 84 & Re 18    &  5 31 45.3 &$-$06 35 58 & HH 83 IRS  & L1641    & 470  \\
295 &          &  5 32 09.1 &$-$05 06 13 & IRAS05329$-$0505 & OMC-3 & 470 \\
131 &          &  5 32 18.9 &$-$08 30 03 &            & Orion    & 470  \\
331 &          &  5 32 40.4 &$-$05 02 42 &            & OMC-3    & 470 \\
269 &          &  5 32 41.7 &$-$05 25 38 &            & M42      & 470 \\
201 & M42-HH1  &  5 32 44.0 &$-$05 23 48 &            & M42      & 470 \\
202 & M42-HH2  &  5 32 44.0 &$-$05 24 40 &            & M42      & 470 \\
205 & M42-HH5  &  5 32 44.4 &$-$05 22 18 &            & M42      & 470 \\
206 & M42-HH6  &  5 32 45.0 &$-$05 22 32 &            & M42      & 470 \\
207 & M42-HH7  &  5 32 45.2 &$-$05 22 43 &            & M42      & 470 \\
401 & HH1/2-NW &  5 32 45.8 &$-$06 31 32 & HH 1/2 VLA1 & L1641   & 470 \\
208 & M42-HH8  &  5 32 46.3 &$-$05 24 15 &            & M42      & 470 \\
209 & M42-HH9  &  5 32 46.4 &$-$05 23 40 &            & M42      & 470 \\
323 & HH 33X   &  5 32 46.5 &$-$06 19 35 &            & L1641    & 470 \\
322 &          &  5 32 46.8 &$-$06 21 45 &            & L1641    & 470 \\
210 & M42-HH10 &  5 32 48.0 &$-$05 22 34 &            & M42      & 470 \\
357 &          &  5 32 48.3 &$-$05 08 03 &            & OMC~3    & 470 \\
 44 &          &  5 32 48.5 &$-$05 12 19 &            & NGC 1976 & 470  \\  
407 &          &  5 32 50.5 &$-$06 01 32 &            & L1641    & 470 \\
 33 &          &  5 32 51.5 &$-$06 19 35 & HH 34 IRS  & L1641    & 470  \\
293 &          &  5 32 53.6 &$-$05 03 08 &            & OMC-3    & 470  \\
 40 & Haro~9a  &  5 32 54.5 &$-$06 20 16 & HH 34 IRS  & L1641    & 470  \\
203 & M42-HH3  &  5 32 54.8 &$-$05 26 51 &            & M42      & 470 \\
385 &          &  5 32 55.0 &$-$05 09 13 &            & OMC 2/3  & 470 \\
204 & M42-HH4  &  5 32 55.2 &$-$05 27 06 &            & M42      & 470 \\
294 &          &  5 32 55.2 &$-$05 05 55 & IRAS05329$-$0505 & OMC 2/3 & 470 \\
384 &          &  5 32 57.7 &$-$05 11 16 &            & OMC 2/3  & 470 \\
 85 & Re 20    &  5 32 58.2 &$-$06 22 15 & HH 34 IRS  & L1641    & 470  \\
383 &          &  5 32 58.7 &$-$05 09 45 &            & OMC 2/3  & 470 \\
126 & Re 21    &  5 33 00.5 &$-$06 24 39 & HH 34 IRS  & L1641    & 470  \\
287 &          &  5 33 01.9 &$-$05 07 08 &            & OMC 2/3    & 470  \\
 34 &          &  5 33 03.7 &$-$06 28 53 & HH 34 IRS  & L1641    & 470 \\
 45 &          &  5 33 06.3 &$-$04 52 43 &            & NGC 1977 & 470  \\
173 &          &  5 33 08.7 &$-$06 34 53 &            & L1641    & 470 \\
134 &          &  5 33 10.1 &$-$06 32 10 &            & L1641    & 470  \\
324 &          &  5 33 14.0 &$-$06 20 25 &            & L1641    & 470 \\
330 &          &  5 33 14.2 &$-$05 06 34 &            & L1641    & 470 \\
 86 & Re 25    &  5 33 14.3 &$-$06 38 04 & HH 34 IRS  & L1641    & 470  \\
222 & Orion Streamers & 5 33 15.6 &$-$06 24 54 & HH 222 VLA & L1641 & 470 \\
 87 & Re 26    &  5 33 17.2 &$-$06 39 21 & HH 34 IRS  & L1641    & 470  \\
 88 & Re 27    &  5 33 18.0 &$-$06 39 46 & HH 34 IRS  & L1641    & 470  \\
310 &          &  5 33 22.2 &$-$05 37 56 &            & L1641    & 470 \\
326 &          &  5 33 23.2 &$-$06 33 55 &            & L1641    & 470 \\
127 & Re 28    &  5 33 24.4 &$-$07 02 08 &            & L1641    & 470  \\
325 &          &  5 33 24.5 &$-$06 31 10 &            & L1641    & 470 \\
  &&&&&& \\ \hline \end{tabular}


\clearpage

\begin{tabular}{|r|p{2.9cm}|r|r|p{2.7cm}|p{2cm}|r|}\hline
\multicolumn{1}{|c|}{HH} &
\multicolumn{1}{c|}{Other} &
\multicolumn{1}{c|}{$\alpha_{1950}$} &
\multicolumn{1}{c|}{$\delta_{1950}$} &
\multicolumn{1}{c|}{Suspected} &
\multicolumn{1}{c|}{Region} &
\multicolumn{1}{c|}{Dist} \\
 & \multicolumn{1}{c|}{designation} & & & \multicolumn{1}{c|}{source} & &
\multicolumn{1}{c|}{$[$pc$]$}  \\ \hline
  &&&&&& \\




327 &          &  5 33 24.6 &$-$06 37 20 &            & L1641    & 470 \\
316 &          &  5 33 28.1 &$-$06 06 44 &            & L1641    & 470 \\
 41 & Haro~3a  &  5 33 34.1 &$-$05 04 40 & IRAS05329$-$0505  & L1641    & 470  \\
308 &          &  5 33 34.4 &$-$06 02 15 &            & L1641    & 470  \\
309 & Re 33         &  5 33 36.2 &$-$05 51 37 &            & L1641    & 470  \\
 42 & Haro~4a  &  5 33 37.3 &$-$05 06 31 & IRAS05329$-$0505           & L1641    & 470  \\
128 & Re 31    &  5 33 40.7 &$-$05 06 28 & IRAS05329$-$0505           & L1641    & 470  \\
307 &          &  5 33 41.0 &$-$06 06 05 &            & L1641    & 470 \\
306 & Re 34    &  5 33 41.5 &$-$06 10 36 &            & L1641    & 470 \\
129 & Re 32    &  5 33 43.3 &$-$05 05 59 &IRAS05329$-$0505            & L1641    & 470  \\
299 &          &  5 33 43.3 &$-$06 21 49 &            & L1641    & 470  \\
296 &          &  5 33 45.2 &$-$06 19 12 &            & L1641    & 470  \\
  3 & Haro~10a &  5 33 45.8 &$-$06 44 53 &            & L1641    & 470  \\
 61 &          &  5 33 47.4 &$-$07 08 51 &            & L1641    & 470  \\
 62 &          &  5 33 47.5 &$-$07 12 51 &            & L1641    & 470  \\
145 &          &  5 33 48.5 &$-$06 48 11 &            & L1641    & 470  \\
297 &          &  5 33 49.3 &$-$06 18 22 &            & L1641    & 470  \\
303 & Re 35/36 &  5 33 52.7 &$-$06 21 24 & IRAS05338$-$0624  & L1641  & 470 \\
  1 & Haro~11a &  5 33 54.5 &$-$06 46 57 & HH 1/2 VLA1 & L1641    & 470  \\
298 &          &  5 33 55.4 &$-$06 23 40 &            & L1641    & 470  \\
144 &          &  5 33 55.4 &$-$06 47 56 & HH 1/2 VLA2 & L1641    & 470  \\
 35 &          &  5 33 56.6 &$-$06 43 40 & V380~Ori   & L1641    & 470  \\
146 &          &  5 33 56.8 &$-$06 50 10 &            & L1641    & 470  \\
305 & Re 37/38/39 & 5 33 57.0 &$-$06 17 32 &          & L1641    & 470  \\
148 &          &  5 33 57.4 &$-$06 45 03 &            & L1641    & 470 \\
147 &          &  5 33 56.9 &$-$06 46 46 & IRAS05339$-$0646 & L1641    & 470 \\
  2 & Haro~12a &  5 33 59.7 &$-$06 49 04 & HH1/2~VLA1 & L1641    & 470  \\
304 & Re 41/42 &  5 34 10.6 &$-$06 16 42 &            & L1641    & 470 \\
301 & Re 43    &  5 34 12.7 &$-$06 23 04 &            & L1641    & 470  \\
130 & Re 45    &  5 34 20.1 &$-$06 51 43 & V380 Ori   & L1641    & 470  \\
 36 &          &  5 34 20.7 &$-$06 46 01 &            & L1641    & 470 \\
 63 &          &  5 34 21.0 &$-$04 27 45 &            & Orion    & 470 \\
302 & Re 44    &  5 34 22.0 &$-$06 22 25 &            & L1641    & 470 \\
285 & AFGL5157/HH5 & 5 34 30.5 & +31 57 17 &          & AFGL 5157 & 1800 \\
281 & AFGL5157/HH1 & 5 34 32.8 & +31 58 28 &          & AFGL 5157 & 1800 \\
282 & AFGL5157/HH2 & 5 34 33.5 & +31 58 19 &          & AFGL 5157 & 1800 \\
292 &          &  5 34 33.7 &$-$06 35 12 & BE Ori     & L1641    & 470 \\
283 & AFGL5157/HH3 & 5 34 34.8 & +31 58 11 &          & AFGL 5157 & 1800 \\
403 &          &  5 34 36.7 &$-$05 54 40 &            & L1641    & 470 \\
284 & AFGL5157/HH4 & 5 34 38.3 & +31 57 51 &          & AFGL 5157 & 1800 \\
404 &          &  5 34 48.7 &$-$05 45 49 &            & L1641    & 470 \\
402 & HH1/2-SE &  5 34 52.0 &$-$07 02 24 & HH 1/2 VLA1 & L1641   & 470 \\
405 & Re 46    &  5 34 57.7 &$-$05 45 20 &            & L1641    & 470 \\
406 &          &  5 35 11.7 &$-$05 41 05 &            & L1641    & 470 \\
 89 & Re 47    &  5 35 21.9 &$-$06 47 47 &            & L1641    & 470  \\
 64 &          &  5 35 22.3 &$-$07 07 12 &            & L1641    & 470  \\
289 &          &  5 35 38.5 &$-$01 45 55 & IRAS05355$-$0146 & Ori-I-2 & 470 \\
 43 & Haro~14a &  5 35 45.4 &$-$07 11 04 & HH 43~IRS1  & L1641    & 470  \\
183 &          &  5 35 52.6 &$-$07 04 06 & V883 Ori   & L1641    & 470 \\
 38 &          &  5 35 56.5 &$-$07 13 18 &            & L1641    & 470  \\
449 &          &  5 36 17.5 &$-$07 14 22 & Haro 4-249 & L1641    & 470 \\
  &&&&&& \\ \hline \end{tabular} 


\clearpage

\begin{tabular}{|r|p{2.9cm}|r|r|p{2.7cm}|p{2cm}|r|}\hline
\multicolumn{1}{|c|}{HH} &
\multicolumn{1}{c|}{Other} &
\multicolumn{1}{c|}{$\alpha_{1950}$} &
\multicolumn{1}{c|}{$\delta_{1950}$} &
\multicolumn{1}{c|}{Suspected} &
\multicolumn{1}{c|}{Region} &
\multicolumn{1}{c|}{Dist} \\
 & \multicolumn{1}{c|}{designation} & & & \multicolumn{1}{c|}{source} & &
\multicolumn{1}{c|}{$[$pc$]$}  \\ \hline
  &&&&&& \\







469 &          &  5 36 54.0 &$-$07 28 03 & Haro 4-255FIR & L1641 & 470 \\
446 &          &  5 36 54.9 &$-$02 35 05 &            & $\sigma$ Ori & 470 \\
470 &          &  5 37 03.8 &$-$07 29 51 & Haro 4-255 & L1641    & 470 \\
444 &          &  5 37 09.0 &$-$02 32 56 & V510 Ori   & $\sigma$ Ori & 470 \\
445 &          &  5 37 09.0 &$-$02 34 50 & A0976-357  & $\sigma$ Ori & 470 \\
447 &          &  5 37 38.1 &$-$02 35 05 & Haro 5-39  & $\sigma$ Ori & 470 \\
 65 &          &  5 37 53.8 &$-$07 26 36 & Re 50 IRS  & L1641    & 470  \\
 66 &          &  5 37 55.0 &$-$02 04 04 &            & L1630    & 470  \\
 67 &          &  5 38 32.6 &$-$01 48 06 &            & L1630    & 470  \\
 90 & Re 51    &  5 38 52.8 &$-$01 11 29 & HH 91 IRS  & L1630    & 470  \\
248 & N2023-HH2     & 5 38 55.6 &$-$02 24 30 &        & NGC 2023 & 470 \\
247 & N2023-HH1,4,5 & 5 39 00.9 &$-$02 18 52 & HH 247 star C & NGC 2023 & 470 \\
249 & N2023-HH3     & 5 39 01.9 &$-$02 25 08 &        & NGC 2023 & 470 \\ 
 68 &          &  5 39 08.7 &$-$06 27 20 &            & Orion    & 470  \\
 69 &          &  5 39 15.6 &$-$06 31 18 &            & Orion    & 470  \\
 91 & Re 52/53 &  5 39 25.9 &$-$01 15 01 & HH 91 IRS  & L1630    & 470  \\
 92 & Re 54    &  5 39 48.9 &$-$01 19 52 &            & L1630    & 470  \\ 
 93 & Re 55    &  5 40 23.8 &$-$01 27 08 &            & L1630    & 470  \\
 94 & Re 56    &  5 40 56.3 &$-$02 34 14 &            & L1630    & 470  \\
212 &          &  5 41 18.9 &$-$01 04 09 &            & L1630    & 470  \\
 95 & Re 57    &  5 41 22.5 &$-$02 39 03 &            & L1630    & 470  \\
175 &          &  5 42 03.0 &  +09 09 00 & IRAS05417+0907 & B35  & 470  \\
 19 &          &  5 43 16.0 &$-$00 06 20 &            & NGC 2068 & 470  \\
 20 &          &  5 43 21.5 &$-$00 04 14 &            & NGC 2068 & 470  \\
 21 &          &  5 43 22.0 &$-$00 05 36 &            & NGC 2068 & 470  \\
 37 & SSWMW 18-37 & 5 43 22.2 &$-$00 06 39 &          & NGC 2068 & 470 \\
 70 &          &  5 43 28.7 &$-$00 06 43 &            & NGC 2068 & 470  \\
 26 &          &  5 43 31.1 &$-$00 15 42 & SSV~59     & NGC 2068 & 470  \\
 25 &          &  5 43 33.2 &$-$00 14 31 & SSV~59     & NGC 2068 & 470  \\
 24 &          &  5 43 36.1 &$-$00 11 02 & SSV~63     & NGC 2068 & 470  \\
 22 &          &  5 43 40.3 &$-$00 06 36 &            & NGC 2068 & 470  \\ 
 23 &          &  5 43 40.9 &$-$00 04 37 & IRAS05436$-$0007  & NGC 2068 & 470  \\
 27 &          &  5 43 49.4 &$-$00 14 45 &            & NGC 2068 & 470  \\
291 &          &  5 44 02.9 &  +20 58 48 &            & CB 34    & 1500 \\
290 &          &  5 44 04.5 &  +20 59 08 &            & CB 34    & 1500 \\
 71 &          &  5 44 46.1 &  +00 39 43 &            & L1630    & 470  \\
471 &          &  5 45 00.6 &  +00 37 47 & LkH$\alpha$ 316 & L1630 & 470 \\
472 &          &  5 45 04.5 &  +00 37 35 &                 & L1630 & 470 \\
473 &          &  5 45 06.2 &  +00 36 59 &                 & L1630 & 470 \\
474 &          &  5 45 11.8 &  +00 38 05 &                 & L1630 & 470 \\
311 &          &  5 47 13.6 &  +02 53 01 & HH 111 VLA & L1617    & 470  \\
110 &          &  5 48 47.8 &  +02 54 09 &            & L1617    & 470  \\
270 &          &  5 48 52.8 & +02 55 22  & HH 270 IRS & L1617    & 470  \\
111 &          &  5 49 07.2 &  +02 47 52 & HH 111 VLA & L1617    & 470  \\
121 &          &  5 49 09.7 &  +02 47 58 & HH 111 VLA & L1617    & 470  \\
116 &          &  5 49 09.7 &  +08 24 40 & IRAS05494+0820 & L1598 & 470  \\
112 &          &  5 49 14.4 &  +02 59 47 &            & L1617    & 470  \\
117 &          &  5 49 39.2 &  +08 15 31 & IRAS05496+0812 & L1598 & 470  \\
118 &          &  5 49 40.0 &  +08 09 34 & IRAS05496+0812 & L1598 & 470  \\
113 &          &  5 50 58.1 &  +02 42 49 & HH 111 VLA  & L1617    & 470  \\
122 &          &  5 52 03.2 &  +01 43 26 &            & L1622    & 470  \\
  &&&&&& \\ \hline \end{tabular}


\clearpage

\begin{tabular}{|r|p{2.9cm}|r|r|p{2.7cm}|p{2cm}|r|}\hline
\multicolumn{1}{|c|}{HH} &
\multicolumn{1}{c|}{Other} &
\multicolumn{1}{c|}{$\alpha_{1950}$} &
\multicolumn{1}{c|}{$\delta_{1950}$} &
\multicolumn{1}{c|}{Suspected} &
\multicolumn{1}{c|}{Region} &
\multicolumn{1}{c|}{Dist} \\
 & \multicolumn{1}{c|}{designation} & & & \multicolumn{1}{c|}{source} & &
\multicolumn{1}{c|}{$[$pc$]$}  \\ \hline
  &&&&&& \\








396 &          &  5 55 03.4 &  +16 32 00 & G192.16-3.82 & Gemini & 2000 \\
397 &          &  5 55 30.7 &  +16 32 31 & G192.16-3.82 & Gemini & 2000 \\
273 & GGD17/HH3 & 6 10 18.3 &$-$06 10 56 &            & L1646    & 830 \\
272 & GGD17/HH2 & 6 10 21.9 &$-$06 10 30 &            & L1646    & 830 \\
271 & GGD17/HH1 & 6 10 23.9 &$-$06 12 10 & Bretz 4    & L1646    & 830 \\
191 &          &  6 11 47.6 &  +13 50 36 & IRS2w      & S269     & 4000 \\
 39 &          &  6 36 21.8 &  +08 54 11 & R~Mon      & Monoceros & 800  \\
124 &          &  6 38 17.0 &  +10 17 58 & IRAS06382+1017 & NGC 2264 & 800  \\
226 & N2264 HH11-6,7   & 6 38 17.2 & +09 42 42 &          & NGC 2264 & 800 \\
225 & N2264 HH14-4,5,6 & 6 38 17.7 & +09 47 09 &          & NGC 2264 & 800 \\
125 &          &  6 38 20.3 &  +09 50 28 &                & NGC 2264 & 800  \\
227 &          &  6 57 07.9 &$-$04 41 58 &            & S287     & 2100 \\
160 & Z CMa jet & 7 01 22.5 &$-$11 28 36 & Z CMa      & S296     & 1150  \\
 72 &          &  7 18 04.5 &$-$23 56 45 & IRAS07180$-$2356 & L1660 & 1500  \\
120 & Re 2     &  8 07 40.0 &$-$35 56 02 & CG30-IRS4  & Gum Nebula & 450  \\
217 & GN08.15.9/HH & 8 15 59.0 &$-$35 43 26 & IRAS08159$-$3543 & Puppis & 3400 \\
188 & Re 4 head & 8 19 28.9 &$-$49 25 12 & IRAS08194$-$4925 & Gum Nebula & 450 \\
246 &          &  8 19 45.7 &$-$49 29 59 &                & Gum Nebula & 450 \\
219 &          &  8 21 09.4 &$-$41 59 05 & IRAS08211$-$4158 & Gum Nebula & 450 \\
 46 &          &  8 24 17.1 &$-$50 50 34 & HH 46/47 IRS   & Gum Nebula & 450  \\
 47 &          &  8 24 22.8 &$-$50 50 00 & HH 46/47 IRS   & Gum Nebula & 450  \\ 
132 &          &  8 33 40.4 &$-$40 28 28 &            & Puppis   & 950  \\
 73 &          &  9 00 26.6 &$-$44 39 25 &            & Vela     & 700  \\
 74 &          &  9 00 28.6 &$-$44 37 59 &            & Vela     & 700  \\
133 &          &  9 09 02.4 &$-$45 18 18 &            & Vela     & 700  \\
 75 &          &  9 09 50.7 &$-$45 30 07 &            & Vela     & 700  \\
171 &          &  9 46 59.2 &$-$54 43 05 &            & Vela     & ?  \\
 48 &          & 11 03 01.9 &$-$77 01 55 & HH 48 IRS  & Cha I    & 150  \\
 49 &          & 11 04 37.4 &$-$77 17 21 & Ced110-IRS4  & Cha I  & 150  \\
 50 &          & 11 04 39.7 &$-$77 16 44 & Ced110-IRS4  & Cha I  & 150  \\
 51 &          & 11 08 21.5 &$-$76 08 01 &            & Cha I    & 150  \\
135 &          & 11 10 05.9 &$-$58 30 14 &            & Carina   & 2700  \\
136 &          & 11 10 09.0 &$-$58 29 44 &            & Carina   & 2700  \\
137 &          & 11 11 49.0 &$-$60 36 17 &            & Carina   & 2200  \\
138 &          & 11 12 01.5 &$-$60 36 35 &            & Carina   & 2200  \\
320 &          & 11 58 58.8 &$-$64 51 29 &            & Sa 136   & 200 \\
321 &          & 11 59 02.4 &$-$64 52 52 & IRAS11590$-$6452 & Sa 136 & 200 \\
274 &          & 12 49 38.7 &$-$76 50 51 & IRAS12496$-$7650 & Cha II & 165 \\
 52 &          & 12 51 27.3 &$-$76 41 40 & IRAS12496$-$7650 & Cha II & 165  \\
 53 &          & 12 51 34.6 &$-$76 41 17 & IRAS12496$-$7650 & Cha II & 165  \\
 54 &          & 12 52 10.0 &$-$76 40 08 & IRAS12496$-$7650 & Cha II & 165  \\
 76 &          & 14 56 32.9 &$-$62 52 20 & IRAS14563$-$6250 & Circinus & 1000  \\
 77 &          & 14 56 42.9 &$-$62 55 53 &                & Circinus & 1000  \\
139 &          & 14 56 51.6 &$-$63 04 59 & vBH 65a        & Circinus & 1000  \\
141 &          & 14 59 14.9 &$-$63 12 09 &                & Circinus & 1000  \\
140 &          & 14 59 15.3 &$-$63 11 05 & vBH 65b        & Circinus & 1000  \\
142 &          & 14 59 17.6 &$-$63 10 41 &                & Circinus & 1000  \\
143 &          & 14 59 19.6 &$-$63 11 51 &                & Circinus & 1000  \\
185 &          & 15 39 50.6 &$-$33 59 46 & IRAS15398$-$3359 & Lupus 1 & 170 \\
186 & Sz 68 jet & 15 42 01.4 &$-$34 08 08 & Sz 68         & Lupus 1 & 170 \\
187 & HG object 1 & 15 42 07.2 &$-$34 08 11 &             & Lupus 1 & 170 \\
  &&&&&& \\ \hline \end{tabular}

\clearpage

\begin{tabular}{|r|p{2.9cm}|r|r|p{2.7cm}|p{2cm}|r|}\hline
\multicolumn{1}{|c|}{HH} &
\multicolumn{1}{c|}{Other} &
\multicolumn{1}{c|}{$\alpha_{1950}$} &
\multicolumn{1}{c|}{$\delta_{1950}$} &
\multicolumn{1}{c|}{Suspected} &
\multicolumn{1}{c|}{Region} &
\multicolumn{1}{c|}{Dist} \\
 & \multicolumn{1}{c|}{designation} & & & \multicolumn{1}{c|}{source} & &
\multicolumn{1}{c|}{$[$pc$]$}  \\ \hline
  &&&&&& \\






 55 &          & 15 53 18.7 &$-$37 42 12 & HH 55 IRS  & Lupus 2  & 150  \\
228 & Th 28 jet & 16 05 08.3 &$-$38 55 16 & Th 28     & Lupus 3  & 170 \\
 78 &          & 16 05 51.3 &$-$38 57 10 &            & Lupus 3  & 170  \\
312 &          & 16 22 54.7 &$-$24 14 01 & SR 4       & Ophiuchus & 160 \\
418 &          & 16 23 11.8 &$-$24 34 15 &            & Ophiuchus & 160 \\
313 &          & 16 23 17.5 &$-$24 16 22 & VLA 1623   & Ophiuchus & 160 \\
419 & C1       & 16 23 22.9 &$-$24 24 06 &            & Ophiuchus & 160 \\
314 &          & 16 23 37.2 &$-$24 34 10 &            & Ophiuchus & 160 \\
 79 &          & 16 23 45.1 &$-$24 13 42 &            & Ophiuchus & 160  \\
224 & WSB 47   & 16 24 15.0 &$-$24 40 31 &            & Ophiuchus & 160 \\
416 & C4S      & 16 24 41.2 &$-$24 42 39 &            & Ophiuchus & 160 \\
417 &          & 16 25 24.4 &$-$24 21 25 &            & Ophiuchus & 160 \\
420 & C5       & 16 25 36.5 &$-$24 30 34 &            & Ophiuchus & 160 \\
 56 &          & 16 28 54.1 &$-$44 48 37 & Re 13      & Norma 1  & 700  \\
 57 &          & 16 28 56.8 &$-$44 49 17 & V346 Nor   & Norma 1  & 700  \\
213 & Re 15/16 & 17 59 26.6 &$-$24 17 16 &            & M8       & 1680 \\
399 &          & 17 59 26.7 &$-$23 04 04 &            & M20 & 1680 \\
180 &          & 18 14 25.2 &$-$19 52 55 &            & Sagittarius & 1700 \\
216 & M16-HH1  & 18 16 05.1 &$-$13 53 03 &            & NGC 6611 & 2300 \\
 80 &          & 18 16 06.9 &$-$20 53 06 & IRAS18162$-$2048 & L291 & 1700  \\
 81 &          & 18 16 07.5 &$-$20 52 23 & IRAS18162$-$2048 & L291 & 1700  \\
476 &   & 18 26 26.3 &  +00 27 12 &                   & Serpens & 310 \\
106 &   & 18 26 46.4 &  +01 12 15 & ESO H$\alpha$ 279 & Serpens & 310  \\
477 &   & 18 27 06.2 &  +01 18 20 &                   & Serpens & 310 \\
460 &   & 18 27 06.4 &  +01 16 20 &                   & Serpens & 310 \\
107 &   & 18 27 15.9 &  +01 23 51 & ESO H$\alpha$ 279 & Serpens & 310  \\
478 &   & 18 27 24.2 &  +01 13 35 &                   & Serpens & 310 \\
458 &   & 18 27 25.7 &  +01 11 38 & SMM 3             & Serpens & 310 \\
456 &   & 18 27 26.9 &  +01 09 10 &                   & Serpens & 310 \\
457 &   & 18 27 27.6 &  +01 08 41 &                   & Serpens & 310 \\
459 &   & 18 27 30.3 &  +01 12 39 & SMM 3             & Serpens & 310 \\
455 &   & 18 27 50.5 &  +01 14 12 & PS 2              & Serpens & 310 \\
108 &   & 18 33 01.7 &$-$00 37 39 & IRAS18331$-$0035    & Serpens & 310  \\
109 &   & 18 33 04.5 &$-$00 36 50 & IRAS18331$-$0035    & Serpens & 310  \\
172 & HHG33.3+0.2 & 18 51 32.7 & +00 28 52 &          & Aquila     & 500 \\
 82 &          & 18 57 53.6 &$-$37 01 36 & S CrA      & Cor.Austr. & 130  \\
101 &          & 18 58 12.3 &$-$37 07 17 & HH 100 IRS & Cor.Austr. & 130  \\
 96 &          & 18 58 18.8 &$-$37 05 11 & HH 100 IRS & Cor.Austr. & 130  \\
 97 &          & 18 58 23.3 &$-$37 04 21 & HH 100 IRS & Cor.Austr. & 130  \\
100 &          & 18 58 26.9 &$-$37 02 59 & HH 100 IRS & Cor.Austr. & 130  \\
 98 &          & 18 58 30.4 &$-$37 01 57 & HH 100 IRS & Cor.Austr. & 130  \\
104 &          & 18 58 36.7 &$-$37 01 37 & R CrA      & Cor.Austr. & 130  \\
 99 &          & 18 58 43.1 &$-$36 59 01 & HH 100 IRS & Cor.Austr. & 130  \\
223 &          & 19 15 45.6 &  +19 06 23 & IRAS19156+1906 & L723 & 300 \\
332 &          & 19 18 05.3 &  +10 54 58 &            & Aquila   & 300 \\
 32 &          & 19 18 07.9 &  +10 56 21 & AS353A     &   Aquila & 300  \\
250 &          & 19 18 51.9 &  +10 46 48 & IRAS19190+1048 & Aquila & 300 \\
221 &          & 19 26 37.5 &  +09 32 24 & Parsamyan 21 & Aquila & 300  \\
119 &          & 19 34 25.8 &  +07 27 24 & B335 IRS   & B335     & 250  \\
387 & V536Aql jet & 19 36 34.8 & +10 23 22 & V536 Aql & Aquila   & 300  \\
165 & 1548C27 jet & 19 40 48.0 & +23 17 09 & 1548C27  & Vulpecula & 2400  \\
  &&&&&& \\ \hline \end{tabular}


\clearpage

\begin{tabular}{|r|p{2.9cm}|r|r|p{2.7cm}|p{2cm}|r|}\hline
\multicolumn{1}{|c|}{HH} &
\multicolumn{1}{c|}{Other} &
\multicolumn{1}{c|}{$\alpha_{1950}$} &
\multicolumn{1}{c|}{$\delta_{1950}$} &
\multicolumn{1}{c|}{Suspected} &
\multicolumn{1}{c|}{Region} &
\multicolumn{1}{c|}{Dist} \\
 & \multicolumn{1}{c|}{designation} & & & \multicolumn{1}{c|}{source} & &
\multicolumn{1}{c|}{$[$pc$]$}  \\ \hline
  &&&&&& \\






365 &             & 19 41 12.0 & +23 22 46 & 1548C27  & Vulpecula & 2400  \\
214 & GN20.18.3/HH & 20 18 21.3 & +37 00 43 & IRAS20183+3700 & Cygnus & 1000 \\ 
425 &          & 20 18 46.0 & +41 12 06  & V1318 Cyg   & Cygnus   & 1000 \\
475 &          & 20 22 53.9 & +42 05 40  &             & Cygnus   & 2000 \\
166 & AFGL 2591 jet & 20 27 36.0 & +40 01 16 &         & IC 1318  & 2000  \\
376 &          & 20 35 36.0 &  +67 43 58 & IRAS20359+6745 & L1152 & 500 \\
375 &          & 20 38 43.2 &  +67 50 39 & IRAS20386+6751 & L1157 & 440 \\
315 &          & 20 45 04.2 &  +67 52 23 & PV Cep     & Cepheus & 500 \\
215 &          & 20 45 23.3 &  +67 46 36 & PV Cep     & L1158 & 500   \\
415 &          & 20 45 34.2 &  +67 49 25 &            & Cepheus & 500 \\
199 &          & 20 55 52.8 &  +77 20 44 & IRAS20582+7724  & L1228    & 300 \\
200 &          & 20 56 11.3 &  +77 19 45 & HH 200 IRS & L1228    & 300 \\
381 &          & 20 56 42.8 & +52 17 18  & IRAS20568+5217 & Cygnus & ?   \\
382 &          & 20 56 52.3 & +52 05 39  &            & Cygnus   &  ?   \\
380 &          & 20 57 39.7 & +52 22 31  &            & Cygnus   &  ?   \\
389 &          & 20 59 32.2 & +50 09 56  & V1331 Cyg  & Cygnus   & 550   \\
424 &          & 20 59 59.3 & +49 40 00  & LkH$\alpha$321B & Cygnus & 550  \\
421 &          & 21 00 16.9 & +49 39 45  & LkH$\alpha$321 & Cygnus &  550 \\
198 & RNO 129  & 21 00 24.0 & +78 11 00  &            & Cepheus   & 300 \\
218 & V645Cyg/HH & 21 38 10.6 & +50 00 43 & V645 Cyg & Cygnus    & 3500 \\ 
103 &          & 21 41 15.8 &  +65 49 55 &            & NGC 7129 & 1000  \\
232 & GGD 32, GM2-32 & 21 41 18.0 &  +65 50 42 &      & NGC 7129 & 1000 \\
242 & HL14 jet & 21 41 29.9 &  +65 52 50 &            & NGC 7129 & 1000 \\
238 & N7129/HH3 & 21 41 31.4 & +65 51 55 &            & NGC 7129 & 1000 \\
237 & N7129/HH2 & 21 41 33.3 & +65 51 37 &            & NGC 7129 & 1000 \\
239 & N7129/HH4 & 21 41 35.2 & +65 52 51 &            & NGC 7129 & 1000 \\
236 & N7129/HH1 & 21 41 50.2 & +65 53 52 &            & NGC 7129 & 1000 \\
167 & LkH$\alpha$234 jet & 21 41 57.6 & +65 53 07 & LkH$\alpha$ 234 & NGC 7129 & 1000  \\
105 &          & 21 42 12.9 &  +65 54 00 &            & NGC 7129 & 1000  \\
234 & GGD 34, GM2-34 & 21 42 20.6 &  +65 54 50 &      & NGC 7129 & 1000 \\
235 & GGD 35, GM2-35 & 21 42 33.5 &  +65 54 38 &      & NGC 7129 & 1000 \\
379 &          & 21 42 59.1 &  +47 18 55 & IRAS21432+4719 & Cygnus &  ?  \\
354 &          & 22 06 01.6 &  +58 57 11 & IRAS22051+5848 & L1165 & 750 \\
251 & S140/HH1 & 22 17 57.4 &  +63 17 50 &            & S140     & 900 \\
252 & S140/HH2 & 22 18 01.1 &  +63 17 32 &            & S140     & 900 \\
253 & S140/HH3 & 22 18 08.4 &  +63 16 38 &            & S140     & 900 \\
254 & S140/HH4 & 22 18 12.7 &  +63 16 09 &            & S140     & 900 \\
363 &          & 22 26 35.0 &  +68 45 39 & IRAS22266+6845 & L1221 & 200\\
398 & LkH$\alpha$233 jet & 22 32 28.3 & +40 24 32 & LkH$\alpha$ 233 & Lacerta & 880\\
149 &          & 22 34 22.0 &  +75 01 32 & IRAS22343+7501 & L1251 & 300  \\
373 &          & 22 35 55.9 &  +74 59 40 &                & L1251 & 300 \\
374 &          & 22 36 33.6 &  +74 51 54 &                & L1251 & 300 \\
364 &          & 22 37 13.5 &  +74 57 29 &                & L1251 & 300 \\
189 & L1251 HH1-2-3 & 22 37 33.7 & +74 55 02 & IRAS22376+7455 & L1251 & 300 \\
168 & GGD 37    & 22 54 04.8 &  +61 45 59 & HW 2       & Ceph A   & 700 \\
169 & GGD 37-NE & 22 54 35.8 &  +61 46 33 & HW 2       & Ceph A   & 700 \\
174 &           & 22 54 59.3 &  +61 45 39 & HW 2       & Ceph A   & 700 \\
377 &           & 23 01 08.4 &  +61 25 53 & IRAS23011+6126 & Ceph E & 700 \\
170 & MWC 1080/HH & 23 15 14.8 & +60 34 19 & MWC 1080  & Cassiopeia & 2200  \\
358 &           & 23 22 42.2 &  +73 56 06  &           & L1262 & 180 \\
359 &           & 23 24 30.7 &  +74 05 57  &           & L1262 & 180 \\
  
  &&&&&& \\ \hline
\end{tabular}
\end{center}

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