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Paper: The Place of Recurrent Novae Among the Symbiotic Stars (Invited speaker)
Volume: 401, RS Ophiuchi (2006) and the Recurrent Nova Phenomenon
Page: 42
Authors: Mikolajewska, J.
Abstract: The observational properties of recurrent novae indicate that they can be divided into two subclasses: systems with a dwarf secondary and systems with a red giant secondary. The second type – which includes RS Oph – bears many similarities to symbiotic stars.
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