1111.6464 (Santi Cassisi)
Santi Cassisi
We briefly review the main physical and structural properties of Very
Low-Mass stars. The most important improvements in the physical inputs required
for the stellar models computations are also discussed. We show some
comparisons with observational measurements concerning both the Color-Magnitude
diagrams, mass-luminosity relations and mass-radius one, in order to disclose
the level of agreement between the present theoretical framework and
observations.
View original:
http://arxiv.org/abs/1111.6464
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