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Thermonuclear Supernova Explosions and Their Remnants: The Case of Tycho

Published online by Cambridge University Press:  19 September 2016

Carles Badenes ,
Eduardo Bravo  and
Kazimierz J. Borkowski
Carles Badenes
Affiliation:
Institut d’Estudis Espacials de Catalunya, Gran Capitá 2-4, 08034 Barcelona, Spain; and, Departament de Física i Enginyeria Nuclear, Universitat Politécnica de Catalunya, Av. Diagonal 647, 08028 Barcelona, Spainbadenes@ieec.fer.es, eduardo.bravo@upc.es
Eduardo Bravo
Affiliation:
Institut d’Estudis Espacials de Catalunya, Gran Capitá 2-4, 08034 Barcelona, Spain; and, Departament de Física i Enginyeria Nuclear, Universitat Politécnica de Catalunya, Av. Diagonal 647, 08028 Barcelona, Spainbadenes@ieec.fer.es, eduardo.bravo@upc.es
Kazimierz J. Borkowski
Affiliation:
Department of Physics, North Carolina State University, Raleigh NC 27695, kborkow@unity.nesu.edu

Summary

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We propose to use the thermal X-ray emission from young supernova remnants (SNRs) originated in Type Ia supernovae (SNe) to extract relevant information concerning the explosion mechanism. We focus on the differences between numerical 1D and 3D explosion calculations, and the impact that these differences could have on the modeling of young SNRs. We use the remnant of the Tycho supernova (SN 1572) as a test case to compare with our predictions, discussing the observational features that allow to accept or discard a given model.

Type
Part III Supernovae: Progenitors/Remnants
Information
International Astronomical Union Colloquium , Volume 192: Cosmic Explosions , 2005 , pp. 233 - 238
Copyright
Copyright © Springer-Verlag 2005

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