Early Pre-Main Sequence Evolution of Low Mass Stars

Details Early Pre-Main Sequence Evolution of Low Mass Stars Early Pre-Main Sequence Evolution of Low Mass Stars

Aug 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ap%26ss.259..279k&link_type=abstract

Astrophysics and Space Science, v. 259, Issue 3, p. 279-284 (1998).

Astronomy and Astrophysics

Astrophysics

2

Scientific paper

Evolution of the gravitational contraction phase of stars having masses
0.3 < M/M&sun; < 1.5 were studied along with deuterium burning.
The equation of state developed by Mihalas et al. (1988) and OPAL
opacity tables were used in our investigation. The theoretical time
lines were compared with observations.

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