Exploració per tema "ISM: supernova remnants"
Ara es mostren els items 3-5 de 5
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The origin of the iron-rich knot in Tycho's supernova remnant
(2017-01-09)
Article
Accés obertX-ray observations of supernova remnants (SNRs) allow us to investigate the chemical inhomogeneity of ejecta, offering unique insight into the nucleosynthesis in supernova explosions. Here we present detailed imaging and ... -
The post-merger magnetized evolution of white dwarf binaries: The double-degenerate channel of sub-Chandrasekhar type Ia supernovae and the formation of magnetized white dwarfs
(2013-08-20)
Article
Accés obertType Ia supernovae (SNe Ia) play a crucial role as standardizable cosmological candles, though the nature of their progenitors is a subject of active investigation. Recent observational and theoretical work has pointed to ... -
The response of a helium white dwarf to an exploding Type Ia supernova
(2015-05-01)
Article
Accés obertWe conduct numerical simulations of the interacting ejecta from an exploding CO white dwarf (WD) with a He WD donor in the double-detonation scenario for Type Ia supernovae (SNe Ia), and study the possibility of exploding ...