English   español  
Por favor, use este identificador para citar o enlazar a este item: http://hdl.handle.net/10261/20560
COMPARTIR / IMPACTO:
Estadísticas
logo share SHARE   Add this article to your Mendeley library MendeleyBASE
Visualizar otros formatos: MARC | Dublin Core | RDF | ORE | MODS | METS | DIDL
Exportar a otros formatos:
Título

Accreting white dwarfs

AutorHernanz, Margarita ; José, Jordi
Fecha de publicación1-feb-2010
ResumenThermonuclear (type Ia) supernovae are explosions in accreting white dwarfs, but the exact scenario leading to these explosions is still unclear. An important step to clarify this point is to understand the behaviour of accreting white dwarfs in close binary systems. The characteristics of the white dwarf (mass, chemical composition, luminosity), the accreted material (chemical composition) and those related with the properties of the binary system (mass accretion rate), are crucial for the further evolution towards the explosion. An analysis of the outcome of accretion and the implications for the growth of the white dwarf towards the Chandrasekhar mass and its thermonuclear explosion is presented.
Descripción10 pages, 2 tables.-- En: "Supernovae: lights in the darkness", October 3-5, 2007, Mao (Menorca), to appear in Proceedings of Science.
Versión del editorhttp://arxiv.org/abs/0809.3914
URIhttp://hdl.handle.net/10261/20560
Aparece en las colecciones: (ICE) Artículos
Ficheros en este ítem:
Fichero Descripción Tamaño Formato  
0809.3914v1.pdf98,66 kBAdobe PDFVista previa
Visualizar/Abrir
Mostrar el registro completo
 


NOTA: Los ítems de Digital.CSIC están protegidos por copyright, con todos los derechos reservados, a menos que se indique lo contrario.