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J/ApJS/110/21     Molecular clouds in Cepheus and Cassiopeia   (Yonekura+ 1997)
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Molecular clouds in Cepheus and Cassiopeia.
    Yonekura Y., Dobashi K., Mizuno A., Ogawa H., Fukui Y.
   <Astrophys. J. Suppl. Ser. 110, 21 (1997)>
   =1997ApJS..110...21Y      (SIMBAD/NED BibCode)
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ADC_Keywords: CO ; Interstellar medium
Keywords: ISM: clouds - ISM: molecules - ISM: structure - radio lines: ISM -
          stars: formation - surveys

Abstract:
    A large-scale ^13CO(J=1-0) survey for nearby molecular clouds was
    performed toward the Cepheus and Cassiopeia regions
    (100{deg}<l<130{deg} and -10{deg}<b<20{deg}) with the velocity
    coverage of -40<V_LSR_<+20km/s by using the two 4m millimeter-wave
    telescopes at Nagoya University. An area of 866 square degrees was
    covered at an 8' grid spacing with a 2.7' beam, and 48750 positions
    were observed. Significant ^13^CO emission (>=1.8K.km/s=3{sigma}) is
    detected at 1015 positions. On the basis of the ^13^CO data, 188
    distinct ^13^CO clouds are identified whose total mass is
    1.0x10^5^M_{sun}_. Physical properties of the ^13^CO clouds such as
    molecular column densities, sizes, and masses are derived for each
    cloud. Astronomical objects associated with the ^13^CO clouds were
    searched for in the literature: 10 H II regions, eight reflection
    nebulae, 23 T Tauri type stars, 28 molecular outflows, and 125 IRAS
    point sources selected as candidates for protostars are likely to be
    associated with the ^13^CO clouds.

File Summary:
--------------------------------------------------------------------------------
  FileName        Lrecl  Records   Explanations
--------------------------------------------------------------------------------
ReadMe             80        .   This file
table1.dat        107      206   A catalog of ^13^CO clouds
table2.dat         61       24   Characteristics of cloud groups
refs.dat          125       33   References
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Byte-by-byte Description of file: table1.dat
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   Bytes Format Units     Label     Explanations
--------------------------------------------------------------------------------
   1-  3  I3    ---       [YDM97]CO Sequential number
                                    ([YDM97] CO NNN in Simbad database)
       4  A1    ---       Note      [bc] Note (1)
   6- 15  A10   ---       Cloud     Cloud name
  17- 22  F6.2  deg       GLON      Galactic longitude
  24- 28  F5.2  deg       GLAT      Galactic latitude
  30- 31  I2    h         RAh       Right ascension (1950) (2)
  33- 34  I2    min       RAm       Right ascension (1950)
  36- 39  F4.1  s         RAs       Right ascension (1950)
      40  A1    ---       DE-       Declination sign
  41- 42  I2    deg       DEd       Declination (1950) (2)
  44- 45  I2    arcmin    DEm       Declination (1950)
  47- 48  I2    arcsec    DEs       Declination (1950)
  50- 52  F3.1  K         TR*       Temperature T^*^_R_(^13^CO)
  54- 56  F3.1  km/s      DV        FWHM line width {DELTA}V(^13^CO)
  58- 62  F5.1  km/s      Vlsr      LSR velocity
  64- 67  F4.1  K.km/s    IntI      Integrated intensity
  69- 72  F4.2  cm-2      tau       Peak optical depth of the ^13^CO line
                                     measured at the peak positions of the
                                     ^13^CO clouds
  74- 77  F4.1  10+21cm-2 N(H2)     H_2_ molecular column density at the peak
                                     position
  79- 81  I3    arcmin    size1     Size (3)
      82  A1    ---       ---       [x]
  83- 85  I3    arcmin    size2     Size (3)
  87- 90  I4    pc        Dist      Adopted distance
      91  A1    ---     n_Dist      [d] Note on Dist (4)
  93- 96  I4    solMass   Mcloud    Molecular mass of the ^13^CO cloud
  98-107  A10   ---     r_Dist      References to the adopted distances (5)
--------------------------------------------------------------------------------
Note (1): b and c indicates the second and third values of the
          observed properties set (T*_R_, {delta}Vc and V_lsr_c)
Note (2): Peak positions of the ^13^CO clouds
Note (3): Sizes of the ^13^CO clouds measured at 1.8K.km/s contours in Fig.1
           (3{sigma})
Note (4): Distances of these clouds were decided by the first step
Note (5): The references are in the ref.dat file
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Byte-by-byte Description of file: table2.dat
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   Bytes Format Units   Label     Explanations
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       1  A1    ---     Group     [CDA] C: Close group D: Distant Group;
                                        A: clouds in Perseus Arm
   2-  3  I2    ---   [YDM97]GCl  Sequential number
                                  ([YDM97] GCl NN in Simbad database)
   5-  7  I3    deg     GLONmin   Minimum galactic longitude
   9- 11  I3    deg     GLONmax   Maximum galactic longitude
  13- 14  I2    deg     GLATmin   Minimum galactic latitude
  16- 17  I2    deg     GLATmax   Maximum galactic latitude
  19- 21  I3    km/s    Vmin      Minimum V_LSR_
  23- 25  I3    km/s    Vmax      Maximum V_LSR_
  27- 30  I4    pc      Dist      Adopted distance of the subgroup
  32- 36  I5    solMass Mass      Total molecular mass of the subgroup
  38- 39  I2    ---     Ncloud    Number of component clouds identified in S3.2.
  41- 55  A15   ---     AssObj    Associated objects
  57- 61  A5    ---   r_Dist      References for adopted distances in refs.dat
--------------------------------------------------------------------------------

Byte-by-byte Description of file: refs.dat
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   Bytes Format Units   Label     Explanations
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   1-  2  I2    ---     Ref       References number
   4- 24  A21   ---     Aut       Author's name
  28- 46  A19   ---     BibCode   Simbad bibcode
  48-125  A78   ---     Com       Comment
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History: Prepared via OCR at CDS.
================================================================================
(End)                          James Marcout,  Patricia Bauer [CDS]  04-May-1998

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