The role of the equation of state in models of very low-mass stars

Details The role of the equation of state in models of very low-mass stars The role of the equation of state in models of very low-mass stars

Jul 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ap%26ss.328..167d&link_type=abstract

Astrophysics and Space Science, Volume 328, Issue 1-2, pp. 167-169

Astronomy and Astrophysics

Astrophysics

Stars, Equation Of State

Scientific paper

The internal structure of low-mass stars turns out to depend critically
on the thermodynamic description of the partial ionization regime. In
this contribution we show the differences among the results obtained
with some of the various equations of state (EOS) available in the
literature.

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