State-Changing Soft X-Ray Sources in M31: White Dwarfs? Neutron Stars? or Black Holes?

Details State-Changing Soft X-Ray Sources in M31: White Dwarfs? Neutron Stars? or Black Holes? State-Changing Soft X-Ray Sources in M31: White Dwarfs? Neutron Stars? or Black Holes?

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009cfdd.confe.176p&link_type=abstract

Chandra's First Decade of Discovery, Proceedings of the conference held 22-25 September, 2009 in Boston, MA. Edited by Scott Wo

Physics

Galaxies

Scientific paper

Our Galaxy and the Magellanic Clouds contain ˜18 well studied supersoft x-ray sources (SSSs). None of these sources has ever been observed in a harder state. Two SSSs in M31 have, however, been observed in quasisoft and/or hard states. We have used Chandra, XMM-Newton, and Swift to document these changes. We present the results and discuss possible models for the sources.

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