Early pre-main sequence evolution of low mass stars
ASTROPHYSICS AND SPACE SCIENCE, vol.259, no.3, pp.279-284, 1998 (SCI-Expanded, Scopus)
- Publication Type: Article / Article
- Volume: 259 Issue: 3
- Publication Date: 1998
- Doi Number: 10.1023/a:1001522620068
- Journal Name: ASTROPHYSICS AND SPACE SCIENCE
- Journal Indexes: Science Citation Index Expanded (SCI-EXPANDED), Scopus
- Page Numbers: pp.279-284
- Middle East Technical University Affiliated: No
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.