J/A+AS/115/81       A CS(2-1) survey of UC HII regions (Bronfman+, 1996)
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A CS(2-1) survey of IRAS point sources with color characteristics of
ultra-compact H II regions
      Bronfman L., Nyman L.-A., May J.
     <Astron. Astrophys. Suppl. Ser. 115, 81 (1996)>
     =1996A&AS..115...81B      (SIMBAD/NED BibCode)
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ADC_Keywords: H II regions ; Radio lines ; Infrared sources

Keywords: Galaxy: structure - infrared: interstellar: continuum -
          interstellar medium : clouds - interstellar medium: H II regions -
          interstellar medium: molecules - radio lines: molecular

Description:
    We have made a complete survey of the CS(2-1) emission toward IRAS
    point sources in the galactic plane. The sources observed were
    selected according to their far infrared (FIR) colors, which are
    characteristic of UC HII regions. They have 25µm/12µm flux
    ratios larger than 3.7 and 60µm/12µm flux ratios larger than
    19.3. The survey covered a region from b=-2deg to b=2deg from l=300deg
    to l=0deg and from l=0deg to l=60deg, and from b=-4deg to b=4deg
    elsewhere. We detected 843 sources out of 1427 sources observed. The
    distributions of detected and undetected sources in a FIR color-color
    diagram show some differences, suggesting that more than one type of
    object is present in our observed sample.

File Summary:

       FileName      Lrecl  Records   Explanations

ReadMe            80        .   This file
table1.dat        48     1449   CS(2-1) survey of UC HII regions


Byte-by-byte Description of file:  table1.dat

   Bytes Format  Units   Label     Explanations

   2-  8  F7.3   deg     GLON      Galactic longitude
  10- 15  F6.3   deg     GLAT      Galactic latitude
  17- 22  F6.1   km/s    VLSR      ? Mean local standard rest velocity
  24- 28  F5.2   K       Tmb       ? Line intensity
  30- 33  F4.1   km/s    DeltaV    ? Line width
  35- 45  A11    ---     IRAS      IRAS source identification
  47- 48  A2     ---    Telescope  [SO*] Telescope used for the observation (1)

Note (1): S= SEST (Swedish-ESO Submillimiter Telescope)
          O= OSO (Onsala Space Observatory)
          *= respective spectrum is of poor quality

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(End)                                             Simona Mei [CDS]   07-Sep-1995