Please use this identifier to cite or link to this item:
http://nopr.niscpr.res.in/handle/123456789/37238| Title: | On the Characteristics of Line Emissions from, Binary X-ray Sources & Supernova Remnants |
| Authors: | Marar, T M K Iyengar, V S Kasturirangan, K Rao, U R |
| Issue Date: | Oct-1979 |
| Publisher: | NISCAIR-CSIR, India |
| Abstract: | X-ray spectroscopy of celestial X-ray sources can yield extremely interesting results on the physical conditions and processes that are responsible for the emission from these sources. Iron line emission at about 6'8 keV from many supernova remnants and X-ray binaries has already been observed by several workers, In this paper we present the available data on iron line emission from Tycho, Cas A and Her X-1 and discuss the implications. |
| Page(s): | 411-413 |
| ISSN: | 0975-105X (Online); 0367-8393 (Print) |
| Appears in Collections: | IJRSP Vol.08(5&6) [October & December 1979] |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| IJRSP 8(5&6) 411-413.pdf | 195.01 kB | Adobe PDF | View/Open |
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