Publication Abstracts
Kumar 1963
Kumar, S.S., 1963: Structure of stars of very low mass. Astrophys. J., 137, 1121-1125, doi:10.1086/147589.
Completely convective models have been constructed for stars of masses 0.09, 0.08, 0.07, 0.06, 0.05, and 0.04 (solar units), taking into account the non-relativistic degeneracy of the stellar material. It is shown that there is a lower limit to the mass of a main-sequence star. The stars with mass less than this limit become completely degenerate stars or "black" dwarfs as a consequence of gravitational contraction, and, therefore, they never go through the normal stellar evolution.
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BibTeX Citation
@article{ku07000g,
author={Kumar, S. S.},
title={Structure of stars of very low mass},
year={1963},
journal={Astrophysical Journal},
volume={137},
pages={1121--1125},
doi={10.1086/147589},
}
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RIS Citation
TY - JOUR ID - ku07000g AU - Kumar, S. S. PY - 1963 TI - Structure of stars of very low mass JA - Astrophys. J. JO - Astrophysical Journal VL - 137 SP - 1121 EP - 1125 DO - 10.1086/147589 ER -
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