Post-mortem Examination of SN1572 from Its Supernova Remnant

Details Post-mortem Examination of SN1572 from Its Supernova Remnant Post-mortem Examination of SN1572 from Its Supernova Remnant

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..342..428b&link_type=abstract

1604-2004: Supernovae as Cosmological Lighthouses, ASP Conference Series, Vol. 342, Proceedings of the conference held 15-19 Jun

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We report preliminary results on the analysis of the X-ray spectrum of the Tycho Supernova Remnant, aimed at determining the explosion mechanism associated with its Type Ia progenitor event, the Supernova of 1572. This work is based on an extensive grid of synthetic spectra generated from hydrodynamic and nonequilibrium ionization calculations of the interaction of several Type Ia explosion models with a uniform ambient medium. The best results are obtained with a 1D delayed detonation model of moderate energy, interacting with an ambient medium of density ρ_{AM} = 2 \cdot 10^{-24} g cm^{-3}.

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