Krishna Swamy, K. S. (1970) Atmospheric structure of cool stars with particle opacity The Astrophysical Journal, 162 . pp. 259-264. ISSN 0004-637X
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Official URL: http://iopscience.iop.org/0004-637X
Abstract
A comparative study of the model atmospheres of cool stars with and without the inclusion of graphite-particle opacity has been made. It is found that the extinction due to graphite particles is appreciable compared with the absorption due to other sources. Therefore, for a discussion of cool stars where particle formation is possible, it is necessary to take into account the opacity due to the particles in the computation of the model atmosphere.
Item Type: | Article |
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Source: | Copyright of this article belongs to American Astronomical Society. |
ID Code: | 87627 |
Deposited On: | 20 Mar 2012 14:32 |
Last Modified: | 20 Mar 2012 14:32 |
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