Circumstellar Interaction, X-ray And Radio Emission, And The Ambient Medium In Young Supernovae

Details Circumstellar Interaction, X-ray And Radio Emission, And The Ambient Medium In Young Supernovae Circumstellar Interaction, X-ray And Radio Emission, And The Ambient Medium In Young Supernovae

Jan 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21343804d&link_type=abstract

American Astronomical Society, AAS Meeting #213, #438.04; Bulletin of the American Astronomical Society, Vol. 41, p.311

Astronomy and Astrophysics

Astronomy

Scientific paper

Using numerical hydrodynamic simulations, we study the interaction of the supernova (SN) shock wave with the surrounding medium in young SNe. Comparison of the X-ray and radio emission resulting from this interaction with the observed data allows for a determination of the structural properties and density profile of the circumstellar medium. Using this we delineate the ambient medium in some well studied SNe such as SN 1993J and SN 1996cr.
Acknowledgements: Several collaborators have contributed to data used in this work and are appropriately listed on the poster. This work is partly supported by Chandra, NSF and STScI grants to VVD at U Chicago.

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