Some observational aspects of R Coronae Borealis Stars

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3366

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DC Field	Value	Language
dc.contributor.author	Kameswara Rao, N	-
dc.date.accessioned	2008-09-04T16:10:00Z	-
dc.date.available	2008-09-04T16:10:00Z	-
dc.date.issued	2008	-
dc.identifier.citation	Werner, Klaus and Rauch, Thomas, eds.,Hydrogen-Deficient Stars, Workshop held at Eberhard Karls University, Astronomical Society of the Pacific Conference Series, Vol. 391, Tubingen, Germany 17 - 21 September, 2007, pp. 25 - 34	en
dc.identifier.isbn	978-1-58381-652-3	-
dc.identifier.uri	http://hdl.handle.net/2248/3366	-
dc.description	Restricted Access	-
dc.description.abstract	Some of the observational aspects related to the evolutionary status and dust production in R Cor Bor stars are discussed. Recent work regarding the surface abundances, stellar winds and evidence for dust production in these high luminosity hydrogen deficient stars are also reviewed. Possibility of the stellar winds being maintained by surface magnetic fields is also considered	en
dc.language.iso	en	en
dc.publisher	Astronomical Society of the Pacific	en
dc.relation.ispartofseries	Astronomical Society of the Pacific Conference Series, Vol. 391	-
dc.relation.uri	http://www.aspbooks.org/a/volumes/article_details/?paper_id=28735	en
dc.rights	© Astronomical Society of the Pacific	en
dc.subject	R Coronae Borealis Stars	en
dc.subject	High luminosity hydrogen deficient stars	en
dc.title	Some observational aspects of R Coronae Borealis Stars	en
dc.type	Article	en
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