Low-mass stars evolutionary models (Baraffe+ 1998)

Details Low-mass stars evolutionary models (Baraffe+ 1998) Low-mass stars evolutionary models (Baraffe+ 1998)

Jul 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ycat..33370403b&link_type=abstract

VizieR On-line Data Catalog: J/A+A/337/403. Originally published in: 1998A&A...337..403B

Physics

5

Stars: Masses, Models: Evolutionary, Photometry

Scientific paper

Physical properties and absolute magnitudes of low-mass stars for different initial metallicity [M/H], helium mass fraction Y and mixing length parameter Lmix: mass (in solar mass), age (in Gyrs) effective temperature (in K), log of gravity (in cgs) and absolute magnitudes. The VRI magnitudes are in the Johnson-Cousins system and the JHK magnitudes in the CIT system. Note that the bolometric magnitude corresponds to M_bol(Sun)=4.64. The lowest mass corresponds to the hydrogen-burning limit. (1 data file).

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