CDROM/APJ/V419/P596  UV Radiation from Evolved Stellar Models. I. (Dorman+ 1993)
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Ultraviolet Radiation from Evolved Stellar Populations I. Models    
      Ben Dorman, Robert T. Rood, & Robert W. O'Connell
      <1993, ApJ, 419, 596>
      =1993ApJ...419..596D
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Description:
  Tables are given for all of the evolutionary tracks in the paper, which
  represent the evolution from the Zero-Age Horizontal Branch to a point 
  either late in the AGB evolution, or in many cases to a point on the 
  white dwarf cooling sequences.

  There are sequences for 8 different compositions. The original grid of
  tracks comprises several tens of thousands of models.  In order to make
  this grid easy to use while not seriously compromising the
  representation of the evolution, much shorter tables have been derived
  for the general user.  The data given here have been derived from these
  original calculations by linear and quadratic interpolation routines.
  For the HB phase, the evolution is represented at a fixed set of core
  helium values. After core exhaustion, the table points are at fixed
  intervals along the evolutionary path.

  The compositions in the tables are denoted as follows:
  
  -----------------------------------------------
  Filename       YHB    [Fe/H]  [O/Fe]    Mc
  -----------------------------------------------
   g14.dat	0.245   -2.26    0.50    0.495
   e64.dat	0.247   -1.48    0.60    0.485
   j63.dat	0.257   -0.47    0.23    0.475
   z22.dat	0.288	+0.00	 0.00	 0.469
   z42.dat	0.292	+0.39	 0.00	 0.464
   z62.dat	0.289	+0.58	 0.00	 0.458
  yz42.dat	0.356	+0.43	 0.00	 0.454
  yz62.dat	0.459	+0.71	 0.00	 0.434
  ----------------------------------------------

  The tables contain header records interspersed with the data records, as
  explained below.  As such, these tables CAN NOT be directly converted to FITS
  ASCII format by processing this document file with the CDS 'tofits' routine.

  The basic format of each composition is as follows:

        Header 1: contains the number, N, of data records to follow, mass,
                  metallicity, oxygen and helium abundance
        Header 2: field names
        Data 1-N: Data records for this track

  The sequence of header 1, header 2, and data records then repeats for the 
  next track until the end of file is reached.
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File Summary:
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File Name    Lrecl    Records    Explanations
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e64.dat         82       1695    e64 composition
g14.dat         82       2014    g14 composition
j63.dat         82       1351    j63 composition
yz42.dat        82       1170    yz42 composition
yz62.dat        82       1101    yz62 composition
z22.dat         82       1408    z22 composition
z42.dat         82       1118    z42 composition
z62.dat         82       1171    z62 composition
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Byte-by-byte Description of file: *.dat (record 1)
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   Bytes Format  Units   Label    Explanations
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   1-15   15X    ---     ---      "Track:   lines "
  16-19   I4     ---     Lines    Number of lines in the track
  20-30   11X    ---     ---      "   Mass =  "
  31-35   F5.3   ---     Mass     Mass
  36-47   12X    ---     ---      "  [Fe/H] =  "
  48-52   F5.2   ---     Fe_H     Metallicity
  53-64   12X    ---     ---      "  [O/Fe] =  "
  65-69   F5.2   ---     O_Fe     Oxygen abundance
  70-76   7X     ---     ---      "  Y =  "
  77-81   F5.3   ---     Y        Helium abundance
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Byte-by-byte Description of file: *.dat (record 2)
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   Bytes Format  Units   Label    Explanations
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   1-82   82X    ---     ---      Head row for data values to follow
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Byte-by-byte Description of file: *.dat (record 3-n)
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   Bytes Format  Units  Label     Explanations
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   1-10   F10.5  Myr    Age       Age since Zero-Age Horizontal Branch (ZAHB)
  11-19   F9.4   ---    Yc        Central helium fraction 
  20-28   F9.4   ---    log_Teff  Effective temperature, Kelvin
  29-37   F9.4   ---    log_L     Surface luminosity, solar units 
  38-46   F9.4   ---    log_g     Surface gravity, cgs units
  47-55   F9.4   ---    log_R     Radius, cm
  56-64	  F9.4   ---    Msh       Mass at peak energy production rate of 
                                    hydrogen burning shell, solar units
  65-73   F9.4   ---    log_Tc    Central Temperature, Kelvin
  74-82	  F9.4   ---    log_rho_c Central density, cgs units
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(End)                                             Lee Brotzman [ADS] 09-May-1994