Theoretical models of very low mass stars and brown dwarfs

Details Theoretical models of very low mass stars and brown dwarfs Theoretical models of very low mass stars and brown dwarfs

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...345..939b&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 345, Oct. 15, 1989, p. 939-958. Research supported by the Alfred P. Sloan F

Astronomy and Astrophysics

Astrophysics

134

Dwarf Stars, Stellar Evolution, Stellar Interiors, Stellar Mass, Stellar Models, Equations Of State, Milky Way Galaxy, Nuclear Reactions, Opacity, Stellar Atmospheres, Stellar Luminosity, Stellar Structure, Stellar Temperature, Tables (Data)

Scientific paper

The results of a new series of stellar evolution calculations are presented for very low mass stars (less than about 0.2 solar mass) and brown dwarfs (less than 0.08 solar mass). The dependence of the effective temperatures, luminosities, radii, etc., on the mixing length, the atmospheric opacities, and the helium fraction are studied along the very low mass star/brown dwarf continuum. Numerical data tables, isochrones, and evolutionary curves of the various observables and structural quantities are presented for seven models of fifteen masses each, between 0.03 solar mass and 0.2 solar mass.

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