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The Origin of X-Ray Emission Lines From SS Cgy
Cataclysmic Variables emission lines SS Cyg dwarf novas
2010/4/9
SS Cyg is a dwarf nova binary star that undergoes frequent large amplitude outburst within a period of 40 days. SS Cyg was observed with the Chandra x-ray telescope in quiescence on 2000 August 24, an...
The Extreme Ultraviolet Emission Lines of Some Cataclysmic Variables at Outburst
Emission lines accretion disks and Cataclysmic Variables
2010/4/9
Using spectral technique, analyses of some astrophysical data from the EUVE satellite in the Extreme Ultraviolet region on accretion disk of some cataclysmic variable were carried out. A number of str...