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Are the models for type Ia supernova progenitors consistent with the properties of supernova remnants?

Autor
Badenes, C.; Bravo, E.; Langer, N.; Hughes, J.P.
Tipus d'activitat
Article en revista
Revista
Astrophysical journal
Data de publicació
2007-06
Volum
662
Número
1
Pàgina inicial
472
Pàgina final
486
DOI
https://doi.org/10.1086/518022 Obrir en finestra nova
Repositori
http://hdl.handle.net/2117/18840 Obrir en finestra nova
URL
http://iopscience.iop.org/0004-637X Obrir en finestra nova
Resum
We explore the relationship between the models for progenitor systems of Type Ia supernovae and the properties of the supernova remnants that evolve after the explosion. Most models for Type Ia progenitors in the single-degenerate scenario predict substantial outflows during the presupernova evolution. Expanding on previous work, we estimate the imprint of these outflows on the structure of the circumstellar medium at the time of the supernova explosion, and the effect that this modified circums...
Citació
Badenes, C. [et al.]. Are the models for type Ia supernova progenitors consistent with the properties of supernova remnants?. "Astrophysical journal", Juny 2007, vol. 662, núm. 1, p. 472-486.
Paraules clau
Binaries: close, Hydrodynamics, Supernova remnants, Supernovae: general, X-rays: ISM
Grup de recerca
GRPFM - Grup de Recerca en Propietats Físiques dels Materials

Participants

  • Badenes, C  (autor)
  • Bravo Guil, Eduardo  (autor)
  • Langer, N  (autor)
  • Hughes, John P.  (autor)