Variable Guillotine Factor Models for Late Type Main Sequence Stars

Five integrations of point source models for late type main sequence stars are presented, the guillotine factor varying with different powers of the density. Radiation pressure has been neglected. A method of applying the models for given luminosity, mass and radius is suggested. Certain transformat...

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Bibliographic Details
Published inMonthly notices of the Royal Astronomical Society Vol. 109; no. 1; pp. 46 - 54
Main Authors Williamson, Ralph E., Duff, G. F. D., Chant, C. A.
Format Journal Article
LanguageEnglish
Published Oxford, UK Oxford University Press 01.02.1949
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Summary:Five integrations of point source models for late type main sequence stars are presented, the guillotine factor varying with different powers of the density. Radiation pressure has been neglected. A method of applying the models for given luminosity, mass and radius is suggested. Certain transformations of the equations into a form convenient for numerical work are included.
Bibliography:istex:43D49EE65B64B1FD005AF78EBBD1C46D435D25CD
ark:/67375/HXZ-WQFM0ZH3-F
ISSN:0035-8711
1365-2966
DOI:10.1093/mnras/109.1.46