Structure and evolution of low-mass stars (Chabrier+ 1997)

Details Structure and evolution of low-mass stars (Chabrier+ 1997) Structure and evolution of low-mass stars (Chabrier+ 1997)

Apr 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997ycat..33271039c&link_type=abstract

VizieR On-line Data Catalog: J/A+A/327/1039. Originally published in: 1997A&A...327.1039C

Physics

Stars: Masses, Models: Evolutionary, Abundances

Scientific paper

Properties of Very Low mass stars for different initial metallicity [M/H] and Helium mass fraction: mass (in solar mass), age (in Gyrs) effective temperature (in K), log of luminosity (in solar L), radius (10^10cm), central temperature Tc (in K) and density RHOc (in gr/cm-3). Abundances of light elements are normalised to their initial abundance (see text). (1 data file).

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