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J/A+AS/118/47       CO observations in spirals (Chini+, 1996)
Dust and CO emission in normal spirals. I. The data
     Chini R., Kruegel E., Lemke R.
    <Astron. Astrophys. Suppl. Ser. 118, 47 (1996)>
    =1996A&AS..118...47C      (SIMBAD/NED BibCode)
ADC_Keywords: Galaxies, radio ; CO ;

Keywords: galaxies: abundances - galaxies: interstellar matter -
          galaxies: spiral - radio continuum: galaxies - radio lines: galaxies

Description:
    We present 1300µm continuum observations and measurements of the
    CO (1-0) and (2-1) emission from the inner regions of 98 normal
    galaxies. The spatial resolution ranges from 11arcsec to 45arcsec.
    The sources come from a complete FIR selected sample of 138 inactive
    spirals with an optical diameter D25≤180arcsec.

File Summary:

       FileName      Lrecl  Records   Explanations

ReadMe            80        .   This file
table1            70       97   Dust emission in normal spirals
table2            75      108   CO emission in normal spirals
tables.tex       112      424   LaTeX version of the tables


Byte-by-byte Description of file: table1

   Bytes Format Units   Label     Explanations

   1-  9  A9    ---     Name      Galaxy name
  11- 12  I2    h       RAh       Right ascension 1950
  14- 15  I2    min     RAm       Right ascension 1950
  17- 20  F4.1  s       RAs       Right ascension 1950
      22  A1    ---     DE-       Declination sign
  23- 24  I2    deg     DEd       Declination 1950
  26- 27  I2    arcmin  DEm       Declination 1950
  29- 30  I2    arcsec  DEs       Declination 1950
  32- 36  F5.1  Mpc     Dist      ? Distance
  39- 42  F4.1  mJy     S11       ? 1300um flux density whithin 11" area,
                                     IRAM 30m telescope (MRT) observations
  44- 47  F4.1  mJy     e_S11     ? rms uncertainty on S11
  50- 54  F5.1  mJy     S24       ? 1300um flux density whithin 24" area,
                                     Swedish ESO Submillimeter Telescope (SEST)
                                     observations
  57- 60  F4.1  mJy     e_S24     ? rms uncertainty on S24
  63- 65  I3    mJy     S70       ? 1300um flux density whithin 70" area,
                                     SEST observations
  67- 70  F4.1  mJy     e_S70     ? rms uncertainty on S70


Byte-by-byte Description of file: table2

   Bytes Format Units   Label     Explanations

   1-  8  A8    ---     Name      Galaxy name
      10  A1    ---     n_Name    A '*' indicates that the spectrum has been
                                   fitted by two Gaussians, and that the
                                   followed data are from the second Gaussian
  12- 15  I4    km/s    Vc1       ? CO(1-0) MRT (24") central velocity
  17- 19  I3    km/s    dVc1      ? CO(1-0) MRT (24") line width
  21- 23  I3    mK      Tmb1      ? CO(1-0) MRT (24") temperature
  27- 30  I4    km/s    Vc2       ? CO(1-0) SEST (45") central velocity
  32- 34  I3    km/s    dVc2      ? CO(1-0) SEST (45") line width
  36- 38  I3    mK      Tmb2      ? CO(1-0) SEST (45") temperature
  40- 43  I4    km/s    Vc3       ? CO(2-1) MRT (12") central velocity
  45- 47  I3    km/s    dVc3      ? CO(2-1) MRT (12") line width
  49- 51  I3    mK      Tmb3      ? CO(2-1) MRT (12") temperature
  53- 56  I4    km/s    Vc4       ? CO(2-1) SEST (24") central velocity
  58- 60  I3    km/s    dVc4      ? CO(2-1) SEST (24") line width
  62- 64  I3    mK      Tmb4      ? CO(2-1) SEST (24") temperature
  67- 70  F4.2  ---     I24"      ? I(2-1)/(1-0) integrated intensities ratio
                                     with the (1-0) lines coming from the 30m
                                     telescope and the other from SEST
  72- 75  F4.2  ---     ISEST     ? I(2-1)/(1-0) integrated intensities ratio
                                     observations refers to 45" in the (1-0)
                                     transition and 24" in (2-1)

(End)                                         Patricia Bauer [CDS]   02-Apr-1996