Para acceder a los documentos con el texto completo, por favor, siga el siguiente enlace: http://hdl.handle.net/2117/19179

Exploring the physics of type Ia supernovae through the x-ray spectra of their remnants
Badenes Montoliu, Carles; Borkowski, K.; Bravo Guil, Eduardo; Hughes, J.P.; Hwang, U.
Universitat Politècnica de Catalunya. Departament de Física i Enginyeria Nuclear; Universitat Politècnica de Catalunya. GAA - Grup d'Astronomia i Astrofísica
We present the results of an ongoing project to use the X-ray observations of Type Ia Supernova Remnants to constrain the physical processes involved in Type Ia Supernova explosions. We use the Tycho Supernova Remnant (SN 1572) as a benchmark case, comparing its observed spectrum with models for the X-ray emission from the shocked ejecta generated from di erent kinds of Type Ia explosions. Both the integrated spectrum of Tycho and the spatial distribution of the Fe and Si emission in the remnant are well reproduced by delayed detonation models with stratified ejecta. All the other Type Ia explosion models fail, including well-mixed deflagrations calculated in three dimensions.
Peer Reviewed
Àrees temàtiques de la UPC::Física::Astronomia i astrofísica
Supernovae
Supernoves
info:eu-repo/semantics/publishedVersion
Artículo
Istituto Nazionale di Astrofisica
         

Mostrar el registro completo del ítem

Documentos relacionados

Otros documentos del mismo autor/a

Badenes Montoliu, Carles; Borkowski, K.J.; Hughes, J.P.; Hwang, U.; Bravo Guil, Eduardo
Badenes Montoliu, Carles; Bravo Guil, Eduardo; Hughes, J.P.
Badenes Montoliu, Carles; Hughes, J.P.; Bravo Guil, Eduardo; Langer, N.