Paradijs, J. ; Vardya, M. S. (1975) Line blanketing and opacity probability distribution function Astrophysics and Space Science, 33 (1). L9-L12. ISSN 0004-640X
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Official URL: http://www.springerlink.com/content/n0866372734829...
Related URL: http://dx.doi.org/10.1007/BF00646027
Abstract
Advantages and limitations of using opacity probability distribution function (OPDF) in computations of model atmospheres for cool stars have been examined. It is concluded that a direct approach, in which a large number of frequency points are taken, may be more appropriate relative to OPDF.
| Item Type: | Article |
|---|---|
| Source: | Copyright of this article belongs to Springer. |
| ID Code: | 57444 |
| Deposited On: | 27 Aug 2011 15:11 |
| Last Modified: | 27 Aug 2011 15:11 |
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