The Place of Recurrent Novae among the Symbiotic Stars

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dc.creatorMikolajewska, Joanna
dc.date2008-03-26
dc.date.accessioned2026-07-07T09:28:24Z
dc.date.available2026-07-07T09:28:24Z
dc.descriptionThe observational properties of recurrent novae indicate that they can be divided into two subclasses:systems with a dwarf and a red giant secondary, respectively. The second type -- which includes RS Oph -- bears many similarities to symbiotic stars.
dc.description10 pages, 3 figures, to appear in the Proceedings of the Meeting: RS Ophiuchi (2006), ed. by Nye Evans, Mike Bode and Tim O'Brien, the Astronomical Society of the Pacific Conference Series
dc.identifierhttps://arxiv.org/abs/0803.3685
dc.identifierhttp://arxiv.org/abs/0803.3685
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/157443
dc.subjectAstrophysics
dc.titleThe Place of Recurrent Novae among the Symbiotic Stars
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