Tarafdar, S. P. ; Vardya, M. S. (1972) On ultraviolet stellar fluxes. III. Importance of H2 Lyman-band absorption in the sun and other stars The Astrophysical Journal, 178 (2). pp. 509-513. ISSN 0004-637X
![[img]](http://repository.ias.ac.in/style/images/fileicons/application_pdf.png)
|
PDF
- Publisher Version
113kB |
Official URL: http://adsabs.harvard.edu/abs/1972ApJ...178..509T
Related URL: http://dx.doi.org/10.1086/151811
Abstract
Lyman-band absorption of H2, when compared with the combined opacity of H, CI, MgI, and SiI, has been found to contribute significantly to the total opacity in the range 912-1900 Å in the solar atmosphere. Inclusion of Lyman-band absorption in the solar model may reduce chromospheric temperature from that given by Gingerich et al. and improve agreement between observed and calculated extreme-ultraviolet and microwave intensities. The Lyman-band absorption may also be important in stars as hot as A0.
| Item Type: | Article |
|---|---|
| Source: | Copyright of this article belongs to American Astronomical Society. |
| ID Code: | 57433 |
| Deposited On: | 27 Aug 2011 15:10 |
| Last Modified: | 18 May 2016 08:49 |
Repository Staff Only: item control page
