Krishna Swamy, K. S. (1977) Equivalent width of molecular lines in stars. III: Lines of Lyman band of H2 and (A-X) Band of CO and SiO in stars Astrophysics and Space Science, 49 (2). pp. 389-398. ISSN 0004-640X
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Official URL: http://www.springerlink.com/content/w24w72p8057745...
Related URL: http://dx.doi.org/10.1007/BF00641988
Abstract
We have calculated the expected equivalent widths of the individual rotational lines of the Lyman band of H2 and (A-X) band of CO and SiO for Main Sequence stars. The results indicate that the lines of H2 should be observable in absorption up to Te≲9000 K. The lines of CO are found to be much weaker than those of H2 lines. A discussion of these results is presented.
| Item Type: | Article |
|---|---|
| Source: | Copyright of this article belongs to Springer-Verlag. |
| ID Code: | 18277 |
| Deposited On: | 17 Nov 2010 12:51 |
| Last Modified: | 04 Jun 2011 09:43 |
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