Chandra HETG and RXTE PCA observations of the old nova V603 Aquilae

Details Chandra HETG and RXTE PCA observations of the old nova V603 Aquilae Chandra HETG and RXTE PCA observations of the old nova V603 Aquilae

Jan 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aspc..261..647m&link_type=abstract

The Physics of Cataclysmic Variables and Related Objects, ASP Conference Proceedings, Vol. 261. Edited by B. T. Gänsicke, K. Beu

Physics

Scientific paper

Previous X-ray observations of V603 Aql, the brightest nova of the 20th century, have shown it to be a bright X-ray source consisting of both high (kT ≥5 keV) and medium (kT ~1 keV) temperature components. We have obtained a 64 ksec observation of this system with Chandra HETG, performed on 2001 April 19/20, and of a series of RXTE PCA observations over the period 2001 April 17--22 for a total of 60 ksec. Here we present preliminary results from these observations.

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