Early pre-main sequence evolution of low mass stars

Date

1998-01-01

Author

Kucuk, I
Kiziloglu, N
Civelek, R

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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.

Subject Keywords

Models, Tables, Cluster, Opacity, State, Equation, Stellar envelopes

URI

https://hdl.handle.net/11511/66544

Journal

ASTROPHYSICS AND SPACE SCIENCE

DOI

https://doi.org/10.1023/a:1001522620068

Collections

Department of Physics, Article

Citation Formats

I. Kucuk, N. Kiziloglu, and R. Civelek, “Early pre-main sequence evolution of low mass stars,” ASTROPHYSICS AND SPACE SCIENCE, vol. 259, no. 3, pp. 279–284, 1998, Accessed: 00, 2020. [Online]. Available: https://hdl.handle.net/11511/66544.