Spectrophotometry of Nova Vulpeculae 1984:1

dc.contributor.author	Shylaja, B. S
dc.date.accessioned	2008-02-26T07:23:38Z
dc.date.available	2008-02-26T07:23:38Z
dc.date.issued	1985
dc.identifier.citation	ESA Scientific and Technical Publications Branch, Recent Results on Cataclysmic Variables. The Importance of IUE and Exosat Results on Cataclysmic Variables and Low-Mass X-Ray Binaries. Proceedings of an ESA workshop held at Remeis Observatory, Bamberg, Germany, April 17 - 19, 1985. pp. 183 – 185	en
dc.identifier.uri	http://hdl.handle.net/2248/2053
dc.description.abstract	The Spectrophotometric observations of the nova Vulpeculae, 1984, # 1 obtained at the Kavalur observatory in September 1984 have been identified and compared with other novae. The nova appears to be in the early decline phase and falls into the category of slow novae.	en
dc.format.extent	213926 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	European Space Agency
dc.relation.uri	http://adsabs.harvard.edu/abs/1985ESASP.236..183S	en
dc.subject	Spectrophotometry	en
dc.subject	Nova Vul 1984
dc.title	Spectrophotometry of Nova Vulpeculae 1984:1	en
dc.type	Article	en