SPIRAL INSTABILITY CAN DRIVE THERMONUCLEAR EXPLOSIONS IN BINARY WHITE DWARF MERGERS

ABSTRACT Thermonuclear, or Type Ia supernovae (SNe Ia), originate from the explosion of carbon-oxygen white dwarfs, and serve as standardizable cosmological candles. However, despite their importance, the nature of the progenitor systems that give rise to SNe Ia has not been hitherto elucidated. Obs...

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Veröffentlicht in:	Astrophysical journal. Letters 2015-02, Vol.800 (1), p.1-6
Hauptverfasser:	Kashyap, Rahul, Fisher, Robert, García-Berro, Enrique, Aznar-Siguán, Gabriela, Ji, Suoqing, Lorén-Aguilar, Pablo
Format:	Artikel
Sprache:	eng
Schlagworte:	ACCRETION DISKS Acquisitions Astronomia i astrofísica ASTROPHYSICS, COSMOLOGY AND ASTRONOMY CARBON Channels COLLISIONS DETONATIONS DISKS ECCENTRIC GRAVITATIONAL INSTABILITIES END Estels nans EVOLUTION Física Hydrodyanamics HYDRODYNAMICS IA SUPERNOVAE Instability Merging OXYGEN PROGENITORS Progenitors (astrophysics) REMNANTS SIMULATIONS Spirals Stability SUPERNOVAE supernovae: general Supernoves THERMONUCLEAR EXPLOSIONS VISIBLE RADIATION WHITE DWARF STARS white dwarfs Àrees temàtiques de la UPC
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