Marar, T. M. K. ; Iyengar, V. S. ; Kasturirangan, K. ; Rao, U. R. (1979) On the characteristics of line emissions from binary X-ray sources and supernova remnants Indian Journal of Radio and Space Physics, 8 . pp. 411-413. ISSN 0367-8393
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Abstract
The paper considers the characteristics of line emissions from binary X-ray sources and supernova remnants. X-ray spectroscopy of celestial X-ray sources can yield useful data on physical conditions and processes responsible for emission from binary X-ray sources; iron line emission at about 6.8 keV from many supernova remnants and X-ray binaries has been observed and the available data on iron line emission from Tycho, Cas A, and Her X-1 are discussed. Iron line emission from supernova remnants including source, distance, luminosity, continuum luminosity, and line feature to continuum ratio are presented, and the iron line intensity vs orbital phase of Her X-1 is depicted.
| Item Type: | Article |
|---|---|
| Source: | Copyright of this article belongs to National Institute of Science Communication and Information Resources. |
| ID Code: | 88302 |
| Deposited On: | 28 Mar 2012 09:49 |
| Last Modified: | 17 Jul 2012 07:55 |
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