Is DZ Andromedae an R Coronae Borealis variable?

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3345

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DC Field	Value	Language
dc.contributor.author	Goswami, A	-
dc.contributor.author	Kameswara Rao, N	-
dc.contributor.author	Lambert, D. L	-
dc.date.accessioned	2008-09-02T15:00:24Z	-
dc.date.available	2008-09-02T15:00:24Z	-
dc.date.issued	1998-08	-
dc.identifier.citation	The Observatory, Vol. 118,No. 1145, pp. 213 - 218	en
dc.identifier.issn	0029 - 7704	-
dc.identifier.uri	http://hdl.handle.net/2248/3345	-
dc.description.abstract	The variable star DZ Andromedae has been suspected to be an R Coronae Borealis variable. Our analysis of a high-resolution spectrum shows that the star has been misclassified: the spectrum resembles that of a K giant. We have determined the stellar parameters - effective temperature, surface gravity, and microturbulence - using model atmosphere. Abundances derived for a range of light elements, many Fe-peak elements, and a few s-process elements indicate a near-solar composition for DZ And.	en
dc.language.iso	en	en
dc.publisher	The Observatory	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1998Obs...118..213G	en
dc.subject	Surface Gravity	en
dc.subject	Micro-turbulence	en
dc.subject	Stellar Parameters	en
dc.title	Is DZ Andromedae an R Coronae Borealis variable?	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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