SN 1006 in Context: From Type Ia Supernova to Remnant

Details SN 1006 in Context: From Type Ia Supernova to Remnant SN 1006 in Context: From Type Ia Supernova to Remnant

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd...9e...3c&link_type=abstract

Supernovae: One Millennium After SN1006, 26th meeting of the IAU, Joint Discussion 9, 17-18 August 2006, Prague, Czech Republic,

Physics

Scientific paper

The evolutionary phases in going from a Type Ia supernova explosion to a 1000 year old remnant are reviewed. The explosion sets up the density and composition structure of the ejecta and can have radiative effects on the surroundings. The early shock interactions may be observable at radio and X-ray wavelengths if the circumstellar density is sufficiently high. The later interaction with the interstellar medium is affected by the collisionless shock physics and hydrodynamic instabilities.

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