Suzaku Observations Of Stellar X-ray Sources And Cataclysmic Variables

Details Suzaku Observations Of Stellar X-ray Sources And Cataclysmic Variables Suzaku Observations Of Stellar X-ray Sources And Cataclysmic Variables

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aas...208.3501m&link_type=abstract

American Astronomical Society Meeting 208, #35.01; Bulletin of the American Astronomical Society, Vol. 38, p.110

Astronomy and Astrophysics

Astronomy

Scientific paper

The broad-band coverage of Suzaku is ideally suited to X-ray observations of cataclysmic variables (CVs), which often have soft and hard components, and prominent Fe Kalpha lines. During the first 6 months of the mission, we have observed the dwarf nova SS Cyg in quiescence and in outburst; the unusual magnetic CV, AE Aqr; and the symbiotic star CH Cyg. I will present early results from all three observations.I will also breifely summarize observations of stellar X-ray sources, notably that of eta Car.

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