Add to ORKGWe 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 Reviewe
Type Ia supernovae (SNe Ia) are thermonuclear explosions of white dwarf stars in close binary system...
We explore the relationship between the models for progenitor systems of Type Ia supernovae and the ...
The remnants of Type Ia supernovae (SNe Ia) can provide important clues about their progenitor histo...
We present the results of an ongoing project to use the X-ray observations of Type Ia Supernova Remn...
We present the results of an ongoing project to use the X-ray observations of Type Ia Supernova Remn...
The relationship between Type Ia supernovae and the thermal X-ray emission from their young supernov...
The supernova remnants (SNRs) left behind by Type Ia supernovae (SNe) provide an excellent opportuni...
The explosion mechanism behind Type Ia supernovae is a matter of continuing debate. The diverse atte...
The explosion mechanism behind Type Ia supernovae is a matter of continuing debate. The diverse atte...
We examine the dynamics and X-ray spectrum of the young Type Ia supernova remnant 0509–67.5 in the c...
We address a new set of models for the spectral analysis of the X-ray emission from young, ejecta-do...
Type Ia supernovae originate from the explosion of carbon–oxygen white dwarfs in binary systems, but...
The well-established Type Ia remnant of Tycho's supernova (SN 1572) reveals discrepant ambient mediu...
We present the first results from an ongoing work aimed to use supernovae remnants to discriminate a...
We explore the relationship between the models for progenitor systems of Type Ia supernovae and the ...
Type Ia supernovae (SNe Ia) are thermonuclear explosions of white dwarf stars in close binary system...
We explore the relationship between the models for progenitor systems of Type Ia supernovae and the ...
The remnants of Type Ia supernovae (SNe Ia) can provide important clues about their progenitor histo...
We present the results of an ongoing project to use the X-ray observations of Type Ia Supernova Remn...
We present the results of an ongoing project to use the X-ray observations of Type Ia Supernova Remn...
The relationship between Type Ia supernovae and the thermal X-ray emission from their young supernov...
The supernova remnants (SNRs) left behind by Type Ia supernovae (SNe) provide an excellent opportuni...
The explosion mechanism behind Type Ia supernovae is a matter of continuing debate. The diverse atte...
The explosion mechanism behind Type Ia supernovae is a matter of continuing debate. The diverse atte...
We examine the dynamics and X-ray spectrum of the young Type Ia supernova remnant 0509–67.5 in the c...
We address a new set of models for the spectral analysis of the X-ray emission from young, ejecta-do...
Type Ia supernovae originate from the explosion of carbon–oxygen white dwarfs in binary systems, but...
The well-established Type Ia remnant of Tycho's supernova (SN 1572) reveals discrepant ambient mediu...
We present the first results from an ongoing work aimed to use supernovae remnants to discriminate a...
We explore the relationship between the models for progenitor systems of Type Ia supernovae and the ...
Type Ia supernovae (SNe Ia) are thermonuclear explosions of white dwarf stars in close binary system...
We explore the relationship between the models for progenitor systems of Type Ia supernovae and the ...
The remnants of Type Ia supernovae (SNe Ia) can provide important clues about their progenitor histo...