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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4296
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dc.contributor.authorMikolajewska, J-
dc.contributor.authorBrandi, E-
dc.contributor.authorGarcia, L-
dc.contributor.authorFerrer, O-
dc.contributor.authorQuiroga, C-
dc.contributor.authorAnupama, G. C-
dc.date.accessioned2009-01-29T14:19:05Z-
dc.date.available2009-01-29T14:19:05Z-
dc.date.issued2002-
dc.identifier.citationMargarita Hernanz and Jordi José., eds., Classical Nova Explosions: International Conference on Classical Nova Explosions. AIP Conference Proceedings, Vol. 637, Sitges, Spain, 20 - 24 May, 2002, pp. 42 - 46en
dc.identifier.urihttp://hdl.handle.net/2248/4296-
dc.description.abstractWe present and discuss a hundred year history of activity of the hot component of RX Pup based on optical photometry and spectroscopy. The outburst evolution of RX Pup resembles that of other symbiotic novae whereas at quiescence the hot component shows activity (high and low activity states) resembling that of symbiotic recurrent novae T CrB and RS Oph.en
dc.publisherAmerican Institute of Physicsen
dc.relation.ispartofseriesAIP Conference Proceedings, Vol. 637-
dc.relation.urihttp://arxiv.org/abs/astro-ph/0210505en
dc.relation.urihttp://dx.doi.org/10.1063/1.1518175en
dc.relation.urihttp://adsabs.harvard.edu/abs/2002AIPC..637...42Men
dc.subjectEvolution of the symbiotic novaen
dc.subjectRX Puppisen
dc.subjectOptical Photometryen
dc.subjectSpectroscopyen
dc.titleEvolution of the symbiotic nova RX Puppisen
dc.typeArticleen
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