Near Infrared Observations of Sakurai's Object during 1998-99

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2867

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DC Field	Value	Language
dc.contributor.author	Kamath, U. S	-
dc.contributor.author	Ashok, N. M	-
dc.date.accessioned	2008-07-24T05:11:02Z	-
dc.date.available	2008-07-24T05:11:02Z	-
dc.date.issued	2002-03	-
dc.identifier.citation	Astrophysics and Space Science, Vol. 279, No. 1-2, pp. 65 - 68	en
dc.identifier.issn	0004-640X	-
dc.identifier.uri	http://hdl.handle.net/2248/2867	-
dc.description	Restricted Access	en
dc.description.abstract	We present new near-infrared observations of Sakurai's Object obtained during 1998-99 when this final helium shell flash object was in the dust condensation phase. The infrared colours have reddened compared to earlier epochs, indicating increased dust condensation. The infrared spectra reveal all the features of a carbon star superposed on a dust continuum.	en
dc.format.extent	48252 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Springer	en
dc.relation.uri	http://www.springerlink.com/content/fwuecb626w63lc86/	en
dc.subject	Stars: AGB and Post- AGB	en
dc.subject	Stars: Individual (V4334 SGR)	en
dc.title	Near Infrared Observations of Sakurai's Object during 1998-99	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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