Vardya, M. S. ; Wildt, Rupert (1960) Molecules and late-type stellar models The Astrophysical Journal, 131 . pp. 448-451. ISSN 0004-637X
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Official URL: http://adsabs.harvard.edu/abs/1960ApJ...131..448V
Related URL: http://dx.doi.org/10.1086/146850
Abstract
A difficulty encountered by Osterbrock, when he tried to identify particular red dwarf stars by interpolating between his models of late-type main-sequence stars, is shown to be alleviated by including the effects produced by hydrogen molecules in the convective zone.
| Item Type: | Article |
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| Source: | Copyright of this article belongs to American Astronomical Society. |
| ID Code: | 57437 |
| Deposited On: | 27 Aug 2011 15:07 |
| Last Modified: | 18 May 2016 08:49 |
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