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VI/65 UV Radiation from Evolved Stellar Pop. I. Models (Dorman+ 1993)
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Ultraviolet Radiation from Evolved Stellar Populations. I. Models
Dorman B., Rood R.T., O'Connell R.W.
<ApJ, 419, 596 (1993)>
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ADC_Keywords: Models, evolutionary
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.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
doc_01 80 114 Introduction
data_01.dat 82 2014 Y=0.245 [Fe/H]=-2.26 [O/Fe]=0.50 Mc=0.495
data_02.dat 82 1695 Y=0.247 [Fe/H]=-1.48 [O/Fe]=0.60 Mc=0.485
data_03.dat 82 1351 Y=0.257 [Fe/H]=-0.47 [O/Fe]=0.23 Mc=0.475
data_04.dat 82 1408 Y=0.288 [Fe/H]=+0.00 [O/Fe]=0.00 Mc=0.469
data_05.dat 82 1118 Y=0.292 [Fe/H]=+0.58 [O/Fe]=0.00 Mc=0.464
data_06.dat 82 1171 Y=0.289 [Fe/H]=+0.58 [O/Fe]=0.00 Mc=0.458
data_07.dat 82 1170 Y=0.356 [Fe/H]=+0.43 [O/Fe]=0.00 Mc=0.454
data_08.dat 82 1101 Y=0.459 [Fe/H]=+0.71 [O/Fe]=0.00 Mc=0.434
data_09.dat 80 68 Generates a FITS file with all models on a Unix station
data_10.dat 76 75 FITS header for all models
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(End) Gail L. Schneider [SSDOO/ADC] 25-Sep-1995