PopStar I: Evolutionary synthesis models (Molla+, 2009)

Details PopStar I: Evolutionary synthesis models (Molla+, 2009) PopStar I: Evolutionary synthesis models (Molla+, 2009)

Jul 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ycat..73980451m&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/398/451. Originally published in: 2009MNRAS.398..451M

Computer Science

Models: Evolutionary, Equivalent Widths, Photometry

Scientific paper

These tables give the complete information of Tables 2-5, 7-9 of the published paper. Each table show the calculations results done for 6 IMFs: * Salpeter (1955ApJ...121..161S) * SAL1, with mlow=0.85 and mup=120M&sun;, and STB, with mlow=1.00 and mup=100M&sun;, * Salpeter (1955ApJ...121..161S) SAL2, * Ferrini et al. (1990A&A...231.391F) FER, * Kroupa et al. (2001MNRAS.322..231K) KRO and * Chabrier (2003ApJ...586L.133C) CHA, with mlow=0.15 and mup=100M&sun;, as IMF mass limits.
For each IMF, calculations are done for 6 metallicities (Z=0.0001, 0.0004, 0.004, 0.008, 0.02 and 0.05) and a variable number of ages from log(age)=5.00 up to log(age)=10.18, the oldest age limit depending on the IMF. Stellar clusters are assumed formed by 1Msun. * Table 2 gives the number of some types of stars which are in each isochrone of a given age and metallicity. * Table 3, as subdirectories z*, gives the HR diagrams obtained with the evolutionary models for a cluster of 1M&sun;. There are a total of 636 tables, 106 for each one of the 6 metallicities Z=0.0001, 0.0004, 0.004, 0.008, 0.02 and 0.05. The 106 tables correspond to 106 different evolutionary ages, which are given in ages.dat file. In each HR table we give the actual mass of each star, the input effective temperature, gravity and luminosity for each star and the modeled effective temperature, gravity and luminosity, the mass loss rate, the errors of effective temperature and gravity given as the difference between the input and the modeled values, a flag (NS= normal star, WC=type C Wolf Rayet star, WN=type N Wolf Rayet star, or PN= planetary nebula) defining the type of star, and 6 columns given the numbers of stars for 6 Initial Mass functions. * Table 4 shows the ejected mechanical energy by the clusters. * Table 5 gives the number of ionizing photons produced by these stellar clusters. * Table 7 gives the information related on Hβ and Hα in emission and absorption (intensities of lines and equivalent widths). * Table 8 and 9 give the magnitudes in the Johnson and SDSS systems, respectively. The values are normalized to a cluster of 1M&sun;.
(14 data files).

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