X-Ray Emission from Core-Collapse Supernovae

Details X-Ray Emission from Core-Collapse Supernovae X-Ray Emission from Core-Collapse Supernovae

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006xmm..prop....6i&link_type=abstract

XMM-Newton Proposal ID #05001702

Physics

Supernovae, Supernova Remnants, Diffuse (Galactic) Emission And Isolated Neutron Stars, Sn 1998S, Xmm-Newton Proposal 05001702

Scientific paper

By studying supernova (SN) shock interactions, physical key parameters such as the circumstellar matter (CSM) density, the mass-loss rate of the progenitor, and temperature of the outgoing and reverse shock can be studied as a function of time. Monitoring of X-ray SNe have allowed us to map the CSM density structure out to large radii (>E18cm) from the sites of the explosions, and to probe the mass-loss rates over significant timescales (10^4 yrs) in the progenitors stellar wind history. Our proposed program will extend this already successful effort by observing known (SNe 2006bp, 2004dj, 1998S) and new (SN 1997eg) X-ray emitting SNe in different stages of their evolution.

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