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Early pre-main sequence evolution of low mass stars
Date
1998-01-01
Author
Kucuk, I
Kiziloglu, N
Civelek, R
Metadata
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This work is licensed under a
Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License
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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