X-Ray Emission Lines from SS Cyg

Details X-Ray Emission Lines from SS Cyg X-Ray Emission Lines from SS Cyg

Oct 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009afrsk..13...20e&link_type=abstract

African Skies, Vol. 13, p. 20-21

Physics

Scientific paper

SS Cyg is a dwarf nova binary star that undergoes frequent large amplitude outbursts within a period of 40 days. SS Cyg was observed with the Chandra X-ray telescope three times between 24 August and 15 September 2000. The spectrum of the source shows strong emission lines of O VII and O VIII in all the three observations. The line strengths for these emission lines for the three observations were measured.
SS Cyg est un système binaire de type nova naine présentant fréquemment de larges pics d'activité s'étalant sur une période de 40 jours. SS Cyg a été observée à trois reprises avec le télescope spatial Chandra entre le 24 Août et le 15 Septembre 2000. Le spectre de la source présente de fortes raies d'émission de type O VII et O VIII dans toutes lesdites observations. L'intensité de ces raies a été mesurée pour toutes les trois observations et les résultats sont présentés ici.

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