Past and future of the central double-degenerate core of Henize 2-428

It has been suggested that Type Ia supernovae (SNe Ia) could be produced in the conditions of the violent merger scenario of the double-degenerate model, in which a thermonuclear explosion could be produced when a double carbon-oxygen white dwarf (CO WD) merges. It has been recently found that the n...

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Veröffentlicht in:	Research in astronomy and astrophysics 2019-04, Vol.19 (4), p.57
Hauptverfasser:	Wu, Dong-Hao, Liu, Dong-Dong, Wang, Bo
Format:	Artikel
Sprache:	eng
Schlagworte:	binaries: close Delay time Gravitational waves Gravity waves Orbits Oxygen Parameter estimation Planetary nebulae Radiation stars: evolution stars: individual Supernovae supernovae: general Thermonuclear explosions White dwarf stars white dwarfs
Online-Zugang:	Volltext
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