A High-Resolution Spectrum of the R Coronae Borealis Star V2552 Ophiuchi

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3698

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DC Field	Value	Language
dc.contributor.author	Kameswara Rao, N	-
dc.contributor.author	Lambert, D. L	-
dc.date.accessioned	2008-09-17T11:37:40Z	-
dc.date.available	2008-09-17T11:37:40Z	-
dc.date.issued	2003-11	-
dc.identifier.citation	The Publications of the Astronomical Society of the Pacific, Vol. 115, No. 813, pp. 1304 - 1307	en
dc.identifier.issn	0004 - 6280	-
dc.identifier.uri	http://hdl.handle.net/2248/3698	-
dc.description.abstract	Photometry and low-resolution spectroscopy have added V2552 Oph to the rare class of R Coronae Borealis variables. We confirm this classification of V2552 Oph through a comparison of our high-resolution optical spectrum of this star and that of R CrB and other F-type members of the class. We show that V2552 Oph most closely resembles Y Mus and FH Sct, stars in which Sr, Y, and Zr are enhanced.	en
dc.language.iso	en	en
dc.publisher	The Astronomical Society of the Pacific	en
dc.relation.uri	http://dx.doi.org/10.1086/379205	en
dc.subject	Stars:Individual (V2552 Ophiuchi)	en
dc.subject	Photometry	en
dc.title	A High-Resolution Spectrum of the R Coronae Borealis Star V2552 Ophiuchi	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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