J/A+AS/104/315 Member of Herbig Ae/Be stellar group (The+ 1994)
A new catalogue of members and candidate members of the Herbig Ae/Be (HAEBE)
stellar group
The P.S., de Winter D., Perez M.R.
<Astron. Astrophys. Suppl. Ser. 104, 315 (1994)>
=1994A&AS..104..315T 1994A&AS..104..315T (SIMBAD/NED RefCode)
ADC_Keywords: Stars, Be ;
Keywords: catalogs - stars: Be - stars: formation - stars: pre-main sequence -
infrared: stars
Description:
An up-to-date catalogue of Herbig Ae/Be (HAEBE) stars and related
objects is listed in five tables, containing 287 objects. Table 1
contains all Ae and Be stars which historically are recognized as true
HAEBE stars or potential candidate members. Table 2 gives the stars of
spectral type Fe, and emission line stars with very uncertain or
unknown spectral type. In Table 3 are given all known Extreme Emission
Line Objects (EELOs), of which most have not been identified to belong
to any specific group. Table 4a and b list other Bep or B[e] stars
with strong IR-excess and unknown spectral type. Table 5 contains the
non-emission line possible young objects. Furthermore, Table 6
contains 35 stars rejected from former published lists of HAEBE stars.
In these tables we are including coordinates, spectral types, visual
magnitudes, ranges in photometric variability and references of
several key publications related to each object. Relevant remarks,
such as the presence of a nebula in the vicinity of an object, are
also given.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
liste2.txt 64 79 Abbreviations of the objects designations
liste3.dat 75 31 Stars of which the optical and IRAS coordinates
are offsetted by ≥ 30"
table1.dat 278 108 Herbig Ae/Be members and candidate members
table2.dat 237 23 F-type PMS stars, potential candidates and
those with unknown spectral type
table3.dat 252 23 Extreme emission line objects (EELOs)
table4a.dat 227 32 Other early type emission line stars with
IR-excess from AIS
table4b.dat 224 87 Other early type emission line stars with
IR-excess from DoH
table5.dat 232 14 Non-emission line early type shell stars and
young stellar candidates
table6.dat 237 35 Emission line stars rejected as Herbig Ae/Be
candidates
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Byte-per-byte Description of file: liste3.dat
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Bytes Format Units Label Explanations
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1- 15 A15 --- Name Optical source name
16- 17 I2 h RAh Right ascension 1950
19- 20 I2 min RAm Right ascension 1950
22- 25 F4.1 s RAs Right ascension 1950
28 A1 --- DE- Declination sign
29- 30 I2 deg DEd Declination 1950
32- 33 I2 arcmin DEm Declination 1950
35- 38 F4.1 arcsec DEs Declination 1950
40- 54 A15 --- IRAS IRAS source
56- 57 I2 h RA.IRASh Right ascension 1950 from IRAS
59- 60 I2 min RA.IRASm Right ascension 1950 from IRAS
62- 65 F4.1 s RA.IRASs Right ascension 1950 from IRAS
67 A1 --- DE.IRAS- Declination sign from IRAS
68- 69 I2 deg DE.IRASd Declination 1950 from IRAS
71- 72 I2 arcmin DE.IRASm Declination 1950 from IRAS
74- 75 I2 arcsec DE.IRASs Declination 1950 from IRAS
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Byte-by-byte Description of file: table*.dat
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Bytes Format Units Label Explanations
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1- 14 A14 --- Name Name of the star
16- 35 A20 --- Cat Catalogue designation (1)
36- 37 I2 h RAh Right ascension 1950 (as obtained from HeB,
the IRAS PSC or SIMBAD)
39- 40 I2 min RAm Right ascension 1950
42- 46 F5.2 s RAs Right ascension 1950
49 A1 --- DE- Declination sign
50- 51 I2 deg DEd Declination 1950 (taken from HeB,
the IRAS PSC or SIMBAD)
53- 54 I2 arcmin DEm Declination 1950
56- 60 F5.2 arcsec DEs []? Declination 1950
61 A1 --- u_DEs [ :*] Uncertainty flag on declination,
* denotes a precision of the order of arcmin
62- 66 F5.2 mag PR []? faintest magnitude of the photometric
range
69- 73 F5.2 mag PR2 []? brightest magnitude of the photometric
range
74- 75 A2 --- n_PR [BRIKpg: ] Type of magnitude (2)
76- 80 F5.2 mag Vmag []? Visual magnitude or faintest visual
magnitude (if range of magnitude)(3)
82- 87 F6.2 mag Vmag2 []? brightest visual magnitude if range of
magnitude
88 A1 --- u_Vmag [ :?d] 'd' indicates a bracketed value
89-111 A23 --- Sp Spectral characteristics (4)
112-156 A45 --- Other Other designation (5)
161-165 A5 --- IRAS IRAS source (6)
167-171 A5 --- Neb Nebula (7)
174-221 A48 --- Rem Remarks (8)
225-284 A60 --- Refs Other references (9)
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Note (1): see details on the various designations in file "liste2.txt"
Note (2): The largest photometric range known from published data.
B, V, R and I indicate that the given magnitudes were obtained
by using filters of the Johnson-Cousins UBVRI system
pg indicates photographically measured magnitudes
K indicates that magnitudes are measured through the 2.2 micrometer
filter of the Johnson JHKLM system.
Note (3): The visual (V) magnitude is given, when the photometric range
listed in the previous column is not visual. However, instead of a
single V value, the range in V is given, whenever it is smaller than
that measured through another passband or determined photographically.
Note (4): The spectral characteristics, such as spectral type,
luminosity class, emission lines (e) in the optical spectrum and the
detection of a shell (sh) spectrum, are given. If several spectral
types are known, they are separated by a slash. Note that the
determination of the spectral type depends on the studied wavelength
region, and is influenced by the variability in the spectral lines. We
also like to mention that a clear distinction between Beq or Bep
objects has not been made. However, in some cases the historically
employed classification is given.
Note (5): The other designations are listed in alphabetic order with a
maximum of three. They are given to avoid confusions with other
identifications, and for the reader's convenience, in cases when
different names are frequently used in the literature. The
abbreviations are explained below. When any confusion exists about the
possible optical identification of an IRAS source, or when different
designations refer to the same optical object, they are separated by
the notation =?, followed by the name of the source.
Note (6): Listed are the confirmed detections of IRAS at or near the
optically identified source. The source of the data is given behind
the abbreviation used which are:
N: No IRAS source
Y: Iras source.
?: IRAS detection hole, see Weintraub 1990
O: Offset between optical- and IRAS-source
Note (7): When it is known that the star is associated with a nebula,
it is indicated by the letter Y (Yes), otherwise by the letter N (No).
For unknown cases, the entries in the column are empty. The references
from which the listed informations are obtained are given behind these
letters.
Note (8): Any special remark found in the literature, such as
near-IR excess, degree of linear polarization, detection of a nearby
companion or of binarity, and the evolutionary status of an object, is
given. The remarks and their references are separated by a dash.
Abbreviations used in the remarks:
Bin: Binary
Cand: Candidate
Class Be: Classical Be-star
Comp: Companion
DST: Double star
Ecl Bin: Eclipsing Binary
Em: Emission
HHO: Herbig-Haro object
HP(I): High (Intrinsic) Pol, 1-3%
L_*: Stellar luminosity
LBV: Luminous Blue Variable
LP(I): Low (Intrinsic) Pol, ≤ 1%
NIRE: Near Infrared Excess
N PN: No Planetary Nebula
Neb: Nebula
Obs Reg: Obscured Region
PN: Planetary Nebula
Pol: Polarization
Poss: Possible
Ref Neb: Reflection Nebula
Reg: Region
Rej: Rejected see sect. 3.3. and Table 2.
Sc: Source
Sp T: Spectral Type
Symb: Symbiotic star
Var: Variable
VHP(I): Very High (Intrinsic) Pol, ≥ 3%
The numbered remarks mean the following:
(1) Sp. char. XY Per w=Aep+sh
(2) Refl. Neb-HeB, DST?-FiM
(3) Neb like star-HeB
(4) High L_*+PN?+Ring Neb-HeB
(5) No IRAS sc-BeC
(6) Triangle Neb-HeB
(7) Bin?-FiM
(8) Close to LSS 3027A=CPD-61 3587-SeE
(9) HAEBE? or B[e]?
(10) in Obs Reg-HeR
(11) N PN+HII Reg-ArC
(12) Neb or Star?-HeB
(13) No IRAS sc-BeC
(14) Two faint Comps-HeR
(15) On edge of small dark cloud-HeB
(16) No IRAS sc-BeC
(17) N PN+Symb?-ArC, LBV?-SoB
(18) Norm. Be?-HeB
The references are indicated by a 3-letter detailed in
the "References in the tables" section below.
Note (9): Additional references of the objects mentioned in other
columns. All the references indicate the published lists where the
star has been quoted and the ones which are used to collect the given
information. The references are indicated by a 3-letter detailed in
the "References in the tables" section below.
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References in the tables:
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(End) Patricia Bauer [CDS] 06-Dec-1993