Nova V4444 Sagittarii 1999 in the early decline and quiescent phases

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4736

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DC Field	Value	Language
dc.contributor.author	Kamath, U. S	-
dc.contributor.author	Ashok, N. M	-
dc.contributor.author	Anupama, G. C	-
dc.date.accessioned	2009-08-07T10:32:19Z	-
dc.date.available	2009-08-07T10:32:19Z	-
dc.date.issued	2008-12	-
dc.identifier.citation	Bulletin of the Astronomical Society of India, Vol. 36, No. 4, pp. 141 - 150	en
dc.identifier.issn	0304-9523	-
dc.identifier.uri	http://hdl.handle.net/2248/4736	-
dc.description.abstract	We present near-infrared and optical spectra of the fast nova V4444 Sagittarii at two single epochs in the early decline phase and unfiltered images obtained in quiescence. Based on this and other available data, we discuss about the nature of this nova, including the possibility of it being a recurrent nova.	en
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://www.ncra.tifr.res.in/~basi/08December/Abstract/361412008.htm	en
dc.rights	© Astronomical Society of India	en
dc.subject	Stars: Novae	en
dc.subject	Cataclysmic Variables	en
dc.subject	Stars: Individual: V4444 Sgr	en
dc.title	Nova V4444 Sagittarii 1999 in the early decline and quiescent phases	en
dc.type	Article	en
Appears in Collections:	BASI Publications IIAP Publications Publications based on data from IAO, Hanle

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