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Thermonuclear Supernova Explosions and Their Remnants: The Case of Tycho

  • Carles Badenes
  • Eduardo Bravo
  • Kazimierz J. Borkowski
Conference paper
Part of the Springer Proceedings in Physics book series (SPPHY, volume 99)

Summary

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.

Keywords

Explosion Mechanism Explosion Model Young Supernova Remnant Thermonuclear Supernova Young SNRs 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer-Verlag Berlin Heidelberg 2005

Authors and Affiliations

  • Carles Badenes
    • 1
    • 2
  • Eduardo Bravo
    • 1
    • 2
  • Kazimierz J. Borkowski
    • 3
  1. 1.Institut d#x2019;Estudis Espacials de CatalunyaBarcelonaSpain
  2. 2.Departament de Física i Enginyeria NuclearUniversitat Politécnica de CatalunyaBarcelonaSpain
  3. 3.Department of PhysicsNorth Carolina State UniversityRaleigh

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