Evolution of Low-Mass Stars. Implications for the Dark Matter Distribution in the Halo

Computer Science

Scientific paper

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Low-Mass Stars, Brown Dwarfs, Dark Matter

Scientific paper

We present up-to-date evolutionary models of low-mass stars, from
M≤0.6 M&sun; down to the hydrogen burning minimum mass, using recent
equation of state and synthetic spectra calculations. Comparison is made
with observed luminosity function for these objects. We also present
implications for the dark-matter distribution in the galactic halo.

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