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SNR-calibrated Type Ia supernova models
Eduardo Bravo, Carles Badenes, Héctor Martínez-Rodríguez
Current Type Ia supernova (SN Ia) models can reproduce most visible+IR+UV observations. In the X-ray band, the determination of elemental abundance ratios in supernova remnants (SN…
White dwarf collisions and the meteoritic Ne-E annomaly
Jordi Isern, Eduardo Bravo
The analysis of noble gases in primitive meteorites has shown the existence of anomalous isotopic abundances when compared with the average Solar System values. In particular it ha…
White Dwarf Collisions, a promising scenario to account for meteoritic anomalies
J. Isern, E. Bravo
It is commonly accepted that collisions between white dwarfs (WD) are rare events that only occur in the dense interior of globular clusters or in the dense outskirts around the ce…
Chandrasekhar and sub-Chandrasekhar models for the X-ray emission of Type Ia supernova remnants (I): Bulk properties
Héctor Martínez-Rodríguez, Carles Badenes, Shiu-Hang Lee +9
Type Ia supernovae originate from the explosion of carbon-oxygen white dwarfs in binary systems, but the exact nature of their progenitors remains elusive. The bulk properties of T…