1. IIA Institutional Repository
  2. IIAP Publications
  3. IIAP Publications
Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2053
Full metadata record
DC FieldValueLanguage
dc.contributor.authorShylaja, B. S-
dc.date.accessioned2008-02-26T07:23:38Z-
dc.date.available2008-02-26T07:23:38Z-
dc.date.issued1985-
dc.identifier.citationESA 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 – 185en
dc.identifier.urihttp://hdl.handle.net/2248/2053-
dc.description.abstractThe 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.extent213926 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherEuropean Space Agency-
dc.relation.urihttp://adsabs.harvard.edu/abs/1985ESASP.236..183Sen
dc.subjectSpectrophotometryen
dc.subjectNova Vul 1984-
dc.titleSpectrophotometry of Nova Vulpeculae 1984:1en
dc.typeArticleen
Appears in Collections:IIAP Publications

Files in This Item:
File Description SizeFormat 
Spectrophotometry of Nova Vulpeculae 1984:1212.72 kBAdobe PDFView/Open
Show simple item record


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.