X-Ray Emission from Supernovae in the SWIFT, Chandra and XMM-Newton Era [Oral Contribution]

Details X-Ray Emission from Supernovae in the SWIFT, Chandra and XMM-Newton Era [Oral Contribution] X-Ray Emission from Supernovae in the SWIFT, Chandra and XMM-Newton Era [Oral Contribution]

Feb 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006sgrb.confe..29i&link_type=abstract

Presented at the KITP Conference: Supernova and Gamma-Ray Burst Remnants, Feb 7, 2006, Kavli Institute for Theoretical Physics,

Physics

Scientific paper

Recent results from high-energy observations of young supernovae (SNe) inthe SWIFT, Chandra, and XMM-Newton era are presented.A coherent picture regarding the CSM structure is slowly emerging fromlong-term X-ray monitoring programs, which indicates that the CSM profilesare strikingly similar for all core-collapse SNe out to large radii (>E18cm) from the sites of the explosions. Establishing the long-term X-raylightcurves also allows to study the spectral evolution from a hardspectral component originating in the forward shock at early times to theemergence of soft X-rays from the reverse shock. Our long-term programs tomonitor the X-ray evolution of decades old SNe such as SNe 1970G, 78K and79C allow, forthe first time, to directly witness the transition from a SN into a SNR.

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