Swift observations of the 2015 outburst of AG Peg - from slow nova to classical symbiotic outburst

Symbiotic stars often contain white dwarfs with quasi-steady shell burning on their surfaces. However, in most symbiotics, the origin of this burning is unclear. In symbiotic slow novae, however, it is linked to a past thermonuclear runaway. In 2015 June, the symbiotic slow nova AG Peg was seen in o...

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Detalles Bibliográficos
Autores principales:	Ramsay, G., Sokoloski, J.L., Luna, G.J.M., Nuñez, N.E.
Formato:	JOUR
Materias:	Accretion, accretion discs Binaries: symbiotic Instabilities Stars: individual: AG Peg
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_00358711_v461_n4_p3599_Ramsay
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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