The disc-eclipsed Supersoft Source in the post-outburst nova V5116 Sgr

Details The disc-eclipsed Supersoft Source in the post-outburst nova V5116 Sgr The disc-eclipsed Supersoft Source in the post-outburst nova V5116 Sgr

Jul 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1248..197s&link_type=abstract

X-RAY ASTRONOMY 2009; PRESENT STATUS, MULTI-WAVELENGTH APPROACH AND FUTURE PERSPECTIVES: Proceedings of the International Confer

Astronomy and Astrophysics

Astronomy

Supernovae, X-Ray Sources (Astronomical), Interstellar Matter, Astronomical Observations, Supernovae, X-Ray Sources, X-Ray Bursts, Interstellar Dust Grains, Diffuse Emission, Infrared Cirrus, Gamma-Ray

Scientific paper

The classical nova V5116 Sgr 2005 No. 2 was observed with XMM-Newton in March 2007 and March 2009. EPIC results of the 2007 observations suggested that the post-outburst supersoft source (SSS) was partially eclipsed by an asymmetric accretion disk in a high inclination system. RGS high resolution spectra show a number of absorption and emission features, some of them evolving along the changing light-curve of this source, in a way that is consistent with the proposed scenario. The last XMM-Newton observation in March 2009 shows only a faint source, harder than in 2007, indicating the turn-off of the SSS.

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