Optical Emission Bands in the Spectrum of the R-Coronae and V854-CENTAURI at Minimum

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2737

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DC Field	Value	Language
dc.contributor.author	Kameswara Rao, N	-
dc.contributor.author	Lambert, D. L	-
dc.date.accessioned	2008-07-18T05:36:04Z	-
dc.date.available	2008-07-18T05:36:04Z	-
dc.date.issued	1993-08-01	-
dc.identifier.citation	Monthly Notices of the Royal Astronomical Society, Vol. 263, No. 3, pp. L27 - L31	en
dc.identifier.issn	0035-8711	-
dc.identifier.uri	http://hdl.handle.net/2248/2737	-
dc.description.abstract	Several unidentified broad emission features, previously seen only in the spectrum of the nebulosity in the Red Rectangle, have been observed in a spectrum of the R CrB star V854 Cen taken in a deep minimum. Similarities and differences between the bands from the two sources are noted. The presence of the bands associated with an R CrB star may suggest that their carrier does not contain hydrogen atoms. Extended red emission seen from the Red Rectangle and probably associated with hydrogenated carbon grains is not present in the spectrum of V854 Cen.	en
dc.format.extent	789106 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Royal Astronomical Society	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1993MNRAS.263L..27K	en
dc.subject	Circumstellar matter	en
dc.subject	Stars: individual: V854 Cen	en
dc.subject	Stars: variables: other	en
dc.subject	ISM: molecules	en
dc.title	Optical Emission Bands in the Spectrum of the R-Coronae and V854-CENTAURI at Minimum	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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