The imprint of a symbiotic binary progenitor on the properties of Kepler's supernova remnant

The imprint of a symbiotic binary progenitor on the properties of Kepler's supernova remnant

We present a model for the type Ia supernova remnant (SNR) of SN 1604, also known as Kepler's SNR. We find that its main features can be explained by a progenitor model of a symbiotic binary consisting of a white dwarf and an AGB donor star with an initial mass of 4-5 M ⊙. The slow, nitrogen-ri...

Disgrifiad llawn

Manylion Llyfryddiaeth
Prif Awduron:	Chiotellis, A, Schure, K, Vink, J
Fformat:	Journal article
Iaith:	English
Cyhoeddwyd:	2012

Eitemau Tebyg

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