The optical spectrum of nova LW Serpentis 1978

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3839

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DC Field	Value	Language
dc.contributor.author	Prabhu, T. P	-
dc.contributor.author	Anupama, G. C	-
dc.date.accessioned	2008-09-23T14:27:29Z	-
dc.date.available	2008-09-23T14:27:29Z	-
dc.date.issued	1987-03	-
dc.identifier.citation	Astrophysics and Space Science , Vol. 131, No. 1 - 2, pp. 479 - 484	en
dc.identifier.issn	0004-640X	-
dc.identifier.uri	http://hdl.handle.net/2248/3839	-
dc.description.abstract	Optical spectroscopic data of the nova LW Serpentis 1978, covering its diffuse-enhanced phase until the onset of the forbidden O I line flash, were obtained at the Vainu Bappu Observatory, Kavalur, between March 10 and April 7, 1978. Emission lines, covering a range of 4000-8700 A at dispersions ranging from 83-675 A/mm, steadily increased during the observation period, with highest increases for H-alpha and O I 8446 A. A mean absorption velocity of -1303 + or - 46 km/s is deduced, and the present spectral evolution is consistent with those of fast novae such as NQ Vul 1976.	en
dc.language.iso	en	en
dc.publisher	Kluwer Academic Publishers	en
dc.relation.uri	http://dx.doi.org/10.1007/BF00668129	en
dc.subject	Novae	en
dc.subject	Radiant flux density	en
dc.subject	Stellar spectrophotometry	en
dc.subject	Visible spectrum	en
dc.subject	Oxygen	en
dc.subject	Spectral energy distribution	en
dc.subject	Spectral resolution	en
dc.subject	Spectrum analysis	en
dc.title	The optical spectrum of nova LW Serpentis 1978	en
dc.type	Article	en
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