Computer Science
Scientific paper
Jan 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..35279139s&link_type=abstract
VizieR On-line Data Catalog: J/A+A/527/A139. Originally published in: 2011A&A...527A.139S
Computer Science
Models: Atmosphere, Binaries: X-Ray
Scientific paper
There are 18 sets of models for six chemical composition (pure hydrogen X=1, pure helium Y=1, and four sets of a solar mix of hydrogen and helium X=0.7374 with various heavy element abundances Z=1, 0.3, 0.1, and 0.01Z&sun;; Z&sun;=0.0134) and three gravities with logg=14.0, 14.3, and 14.6 (g in units cm/s2^). Each of these 18 sets is also characterized by the Eddington temperature at the surface, neutron star radius (computed for the assumed mass 1.4M&sun;), and the redshift, as detailed in set.dat file.
tablea1.dat, for each of the 18 sets there are 20 lines of data (for 20 values of l and corresponding effective temperatures) containing color corrections computed by five different procedures described in the paper. The product of dilution factor and fc4^ are also given for the procedures 1-3. They are computed from the models presented in tablea2.dat.
For each set, 20 models are computed for relative luminosities (in units of Eddnington) l=L/L_Edd = 0.001, 0.003, 0.01, 0.03, 0.05, 0.07, 0.1, 0.15, 0.2, 0.3, 0.4, 0.5, 0.6, 0.7, 0.75, 0.8, 0.85, 0.9, 0.95, 0.98.
(3 data files).
Poutanen Juri
Suleimanov Valery
Werner Kirstin
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