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Thermal X-ray emission from shocked ejecta in Type Ia supernova remnants. II : parameters affecting the spectrum

Autor
Badenes, C.; Borkowski, K.; Bravo, E.
Tipus d'activitat
Article en revista
Revista
Astrophysical journal
Data de publicació
2005-05
Volum
624
Número
1
Pàgina inicial
198
Pàgina final
212
DOI
https://doi.org/10.1086/428829 Obrir en finestra nova
Repositori
http://hdl.handle.net/2117/18849 Obrir en finestra nova
URL
http://iopscience.iop.org/0004-637X/624/1/198/ Obrir en finestra nova
Resum
The supernova remnants (SNRs) left behind by Type Ia supernovae (SNe) provide an excellent opportunity for the study of these enigmatic objects. In a previous work we showed that it is possible to use the X-ray spectra of young Type Ia SNRs to explore the physics of Type Ia SNe and identify the relevant mechanism underlying these explosions. Our simulation technique is based on hydrodynamic and nonequilibrium ionization calculations of the interaction of a grid of Type Ia explosion models with t...
Citació
Badenes, C.; Borkowski, K.; Bravo, E. Thermal X-ray emission from shocked ejecta in Type Ia supernova remnants. II. Parameters affecting the spectrum. "Astrophysical journal", Maig 2005, vol. 624, núm. 1, p. 198-212.
Paraules clau
Hydrodynamics, Ism: General, Nuclear Reactions, Nucleosynthesis, Abundances, Supernova Remnants, Supernovae: General, X-rays: Ism
Grup de recerca
GRPFM - Grup de Recerca en Propietats Físiques dels Materials

Participants