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Progenitor's Signatures in Type Ia Supernova Remnants

Published online by Cambridge University Press:  17 January 2013

A. Chiotellis ,
D. Kosenko ,
K. M. Schure  and
J. Vink
A. Chiotellis
Affiliation:
Sterrenkundig Instituut Utrecht, Postbus 80000, NL-3508TA, Utrecht, the Netherlands email: a.chiotellis@astro-uu.nl
D. Kosenko
Affiliation:
Sterrenkundig Instituut Utrecht, Postbus 80000, NL-3508TA, Utrecht, the Netherlands email: a.chiotellis@astro-uu.nl
K. M. Schure
Affiliation:
Sterrenkundig Instituut Utrecht, Postbus 80000, NL-3508TA, Utrecht, the Netherlands email: a.chiotellis@astro-uu.nl Department of Physics, University of Oxford, Clarendon Laboratory, Parks Road, Oxford OX1 3PU, United Kingdom
J. Vink
Affiliation:
Sterrenkundig Instituut Utrecht, Postbus 80000, NL-3508TA, Utrecht, the Netherlands email: a.chiotellis@astro-uu.nl
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Abstract

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The remnants of Type Ia supernovae (SNe Ia) can provide important clues about their progenitor histories. We discuss two well-observed supernova remnants (SNRs) that are believed to have resulted from SNe Ia, and use various tools to shed light on the possible progenitor histories. We find that Kepler's SNR is consistent with a symbiotic binary progenitor consisting of a white dwarf and an AGB star. Our hydrosimulations can reproduce the observed kinematic and morphological properties. For Tycho's remnant we use the characteristics of the X-ray spectrum and kinematics to show that the ejecta has likely interacted with dense circumstellar gas.

Keywords

supernova remnants — supernovae: individual (SN 1604, SN 1572) — binaries: symbiotic
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Issue S281: Binary Paths to Type Ia Supernovae Explosions , July 2011 , pp. 331 - 334
Copyright
Copyright © International Astronomical Union 2013

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