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J/ApJS/89/189       IRAS PSC new OH/IR stars. III. (Chengalur+ 1993)
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New OH/IR stars from color-selected IRAS sources.  III. A complete survey
     Chengalur J.N., Lewis B.M., Eder J., Terzian Y.
    <Astrophys. J. Suppl. Ser. 89, 189 (1993)>
    =1993ApJS...89..189C      (SIMBAD/NED BibCode)
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ADC_Keywords: Infrared sources ; Radio lines
Keywords: infrared: stars - radio lines: stars - stars: AGB and post-AGB -
          surveys

Abstract:
    We present the results of 1612MHz observations conducted at the
    Arecibo Observatory of 571 color-selected sources from the IRAS Point
    Source Catalog. Of these sources we detect 132, 113 for the first
    time. This is the third part of an Arecibo survey of color-selected
    IRAS sources. The earlier two parts together detected a total of 268
    sources of 1612MHz emission.
    An analysis of the properties of the OH/IR stars detected in all three
    parts of the survey is included. In particular we compute the limiting
    1612MHz peak flux of the entire survey to be ~40mJy.
    The correlation between the IRAS infrared fluxes and the 1612MHz flux
    of the 132 sources detected in part III of the survey is smaller than
    that found in the earlier parts of the survey. This is to be expected
    from the intrinsic variability of OH/IR stars and the longer time gap
    between the 1612MHz observations and the IRAS measurements.
    We identify a subset of 54 stars as being near the tangent point of
    the galactic rotation curve. Using the kinematical distances to these
    stars we find that the efficiency of momentum transfer varies
    exponentially with the (25-12){mu}m color, consistent with the stellar
    outflow being driven by radiation pressure. Further the IR pump
    efficiency increases with increasing optical depth of the
    circumstellar shell, as expected for radiative pumping.
    The bolometric luminosity function is found to decrease sharply above
    L_Bol_=5600L_{sun}_, and the 1612MHz luminosity function shows a
    corresponding falloff above L_1612_=1.8x10^-8^L_{sun}_. We also find
    direct confirmation of the expectation that sources with large
    expansion velocity are more luminous than sources with small expansion
    velocity.

File Summary:
--------------------------------------------------------------------------------
  FileName      Lrecl  Records   Explanations
--------------------------------------------------------------------------------
ReadMe             80        .   This file
table1            125      132   Detections
table2             41      439   Non-detections
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See also:
  II/125        : IRAS Point Source Catalogue, Version 2.0 (IPAC 1986)
  J/A+AS/90/327 : IRAS Point Source 1612MHz OH survey (te Lintel Hekkert+ 1991)

Byte-by-byte Description of file: table1
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   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1- 10  A10   ---     IRAS      IRAS name
      11  A1    ---   m_IRAS      Multiplicity index on IRAS name
      12  A1    ---   n_IRAS      [*] Note on IRAS name (1)
  14- 18  F5.1  deg     GLON      Galactic longitude
  20- 24  F5.1  deg     GLAT      Galactic latitude
  26- 27  I2    h       RAh       Right ascension (1950)
  28- 29  I2    min     RAm       Right ascension (1950)
  30- 33  F4.1  s       RAs       Right ascension (1950)
      34  A1    ---     DE-       Declination sign
  35- 36  I2    deg     DEd       Declination (1950)
  37- 38  I2    arcmin  DEm       Declination (1950)
  39- 40  I2    arcsec  DEs       Declination (1950)
  42- 49  F8.1 mJy.km/s S1612MHz  Total integrated 1612MHz flux
  51- 58  F8.1 mJy.km/s S1612-l   Integrated 1612MHz flux in the low-velocity
                                   half of the spectrum
  60- 67  F8.1 mJy.km/s S1612-h   ? Integrated 1612MHz flux in the high-velocity
                                     half of the spectrum
  69- 72  F4.1  km/s    DV(100)   ? Velocity separation between the half-power
                                     points of the two peaks in the line profile
                                     {DELTA}V_100_
  74- 77  F4.1  km/s    DV(50)    ? Velocity separation between the half-power
                                     points of the two peaks in the line profile
                                     {DELTA}V_50_
      78  A1    ---   u_DV(50)    [)] Uncertainty flag on DV(50).
  79- 84  F6.1  km/s    Vl        LSR velocity of the low-velocity peak
  86- 90  F5.1  km/s    Vh        ? LSR velocity of the high-velocity peak
  92- 97  F6.1  km/s    <V>       Systemic LSR velocity
  99-105  F7.4  mag     (25-12)   ? (25-12){mu}m infrared color
 107-113  F7.4  mag     (60-25)   ? (60-25){mu}m infrared color
 115-129  A15   ---     Name      Other name, if the source corresponds to one
                                   known before the IRAS survey
--------------------------------------------------------------------------------
Note (1): *: OH source not listed in the compilation by
              te Lintel Hekkert et al., 1989A&AS...78..399T
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Byte-by-byte Description of file: table2
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   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1- 10  A10   ---     IRAS      IRAS name
  12- 16  F5.1  deg     GLON      Galactic longitude
  18- 22  F5.1  deg     GLAT      Galactic latitude
  24- 30  F7.4  mag     (12-25)   (12-25){mu}m infrared color
  32- 38  F7.4  mag     (60-25)   (60-25){mu}m infrared color
--------------------------------------------------------------------------------

History: Prepared via OCR at CDS.

References:
   Eder J. et al., Paper I, =1988ApJS...66..183E
   Lewis et al., Paper II,  =1990ApJ...362..634
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(End)                           James Marcout, Patricia Bauer [CDS]  28-Nov-1996

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