J/A+A/447/609     1.2mm continuum observations in rho Oph cloud  (Stanke+, 2006)
An unbiased search for the signatures of protostars in the ρ Ophiuchi
molecular cloud. II. Millimetre continuum observations.
    Stanke T., Smith M.D., Gredel R., Khanzadyan T.
   <Astron. Astrophys., 447, 609-622 (2006)>
   =2006A&A...447..609S 2006A&A...447..609S
ADC_Keywords: Interstellar medium ; Molecular clouds ; Millimetric/submm sources
Keywords: stars: formation - ISM: clouds -
          ISM: individual objects: rho Ophiuchi - ISM: structure
Abstract:
    We have performed a wide field survey for dust sources at
    1.2-millimetres in the rho Ophiuchi molecular cloud, covering more
    than 1 square degree in an unbiased fashion. We detect a number of
    previously unknown sources, ranging from extended cores over compact,
    starless cores to envelopes surrounding young stellar objects of
    Class 0, Class I, and Class II type. We analyse the mass distribution,
    spatial distribution and the potential equilibrium of the cores.
Description:
    The observations were carried out using the SIMBA bolometer array at
    the SEST telescope on La Silla/Chile during an observing run lasting
    from 2002 July 7 to 12. SIMBA is a 37-channel bolometer array,
    operating at 1.2mm, and provides a HPBW of ∼24" (as measured on maps
    of Uranus).
File Summary:
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 FileName   Lrecl  Records   Explanations
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ReadMe         80        .   This file
tablea1.dat   149      143   List of 1.2 mm sources found in our survey.
notes.dat      80      252   Individual notes
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See also:
   J/A+A/426/171 : H2 flows in rho Ophiuchi A (Khanzadyan+, 2004)
Byte-by-byte Description of file: tablea1.dat
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   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1-  6  A6    ---     [SSG2006] Sequential number, MMSNNN (1)
   8-  9  I2    h       RAh       Right ascension (J2000)
  11- 12  I2    min     RAm       Right ascension (J2000)
  14- 18  F5.2  s       RAs       Right ascension (J2000)
      19  A1    ---     DE-       Declination sign (J2000)
  20- 21  I2    deg     DEd       Declination (J2000)
  23- 24  I2    arcmin  DEm       Declination (J2000)
  26- 27  I2    arcsec  DEs       Declination (J2000)
  29- 33  I5    mJy     Fint      Integrated source flux
  35- 38  I4    mJy     Fpeaka    Peak flux for maximum pixel value inside an
                                   ellipse defined by the minor and major axes
                                   of a Gauss-fit to the source
  40- 43  I4    mJy     Fpeakb    ? Peak flux as Fpeaka, but using only the
                                     wavelet scales from where on the source is
                                     detected first
      45  A1    ---     ---       [(]
      46  I1    ---     1Det      [1/4]? Wavelet scale from where on the source
                                          is detected first
      47  A1    ---     ---       [)]
  49- 52  I4    mJy     Fpeakc    Peak flux after re-binning according to the
                                   source minor axis
  54- 57  I4    mJy     Fpeakd    Peak flux of the composite Gaussian model for
                                   the source
  59- 61  I3    arcsec  FWHMmaj   Major axis of a single Gaussian fit to
                                   the source
  63- 65  I3    arcsec  FWHMmin   Minor axis of a single Gaussian fit to
                                   the source
  67- 69  I3    deg     PA        [-90/90] Position angle of the source major
                                   axis in degrees east of north
  71- 86  A16   ---     MAN98     Cross-identifications to sources identified by
                                   Motte et al., 1998A&A...336..150M 1998A&A...336..150M (2)
  88-112  A25   ---     [JWM2000] Cross-identifications to sources identified by
                                   Johnstone et al., 2000ApJ...545..327J 2000ApJ...545..327J
                                   [JWM2000] SMM JHHMMm-DDMMa in Simbad (2)
 114-149  A36   ---     Com       Comment on association with known YSOs is
                                   given (3)
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Note (1): The sources are listed in the order they were identified by the
          wavelet decomposition plus clumpfind technique.
Note (2): A long dash (---) means that the source is outside the respective
          survey area, and "n.i.'' labels features which are visible in the
          respective survey, but not identified as a separate feature.
          Cross-identifications given in parentheses mean that a feature found
          here is a part of a feature noted by Motte et al. 1998A&A...336..150M 1998A&A...336..150M
          or Johnstone et al., 2000ApJ...545..327J 2000ApJ...545..327J.
Note (3): Apparently starless features are marked as "sl".
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Byte-by-byte Description of file: notes.dat
--------------------------------------------------------------------------------
   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1-  6  A6    ---     [SSG2006] Sequential number, MMSNNN
   8- 80  A73   ---     Note      Text of the note
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History:
    From electronic version of the journal
(End)                                      Patricia Vannier [CDS]    16-May-2006