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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2790
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dc.contributor.authorKamath, U. S-
dc.contributor.authorAnupama, G. C-
dc.date.accessioned2008-07-22T06:11:37Z-
dc.date.available2008-07-22T06:11:37Z-
dc.date.issued2002-09-
dc.identifier.citationBASI, Vol. 30, No. 3, pp. 679 - 681en
dc.identifier.urihttp://hdl.handle.net/2248/2790-
dc.description.abstractV445 Puppis is a peculiar variable which had a nova-like eruption in December 2000. The early spectra did not show any emission lines of hydrogen or helium. Fe II lines were very dominant during this phase. We present optical spectra of the early-decline phase of V 445 Pup obtained from the Vainu Bappu Observatory during Feb-April 2001.en
dc.format.extent83695 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectStars-Variable-Nova-likeen
dc.subjectSpectroscopy-Opticalen
dc.subjectStars-Individual-V445 Puppisen
dc.titleOptical Spectroscopy of the nova-like variable V 445 Puppisen
dc.typeArticleen
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