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Early Pre-Main Sequence Evolution of Low Mass Stars
Authors:Ibrahim Küçük  Nilgün Kiziloglu  Rikkat Civelek
Institution:(1) Department of Physics, Erciyes University, 38039 Kayseri, Turkey;(2) Department of Physics, Middle East Technical University, 06531 Ankara, Turkey
Abstract:Evolution of the gravitational contraction phase of stars having masses 0.3 < M/M⊙ < 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. This revised version was published online in July 2006 with corrections to the Cover Date.
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