The emission-line spectrum of the hot R Coronae Borealis star MV SGR

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2814

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DC Field	Value	Language
dc.contributor.author	Pandey, G	-
dc.contributor.author	Kameswara Rao, N	-
dc.contributor.author	Lambert, D. L	-
dc.date.accessioned	2008-07-22T11:35:42Z	-
dc.date.available	2008-07-22T11:35:42Z	-
dc.date.issued	1996-10	-
dc.identifier.citation	Monthly Notices of the Royal Astronomical Society, Vol. 282, No. 3, pp. 889 - 899	en
dc.identifier.issn	0035-8711	-
dc.identifier.uri	http://hdl.handle.net/2248/2814	-
dc.description.abstract	Spectra of MV Sgr obtained at CTIO in 1992 May show many emission lines in the red. Most of the emission lines show two components with a minimum centred at the stellar velocity. Species represented include H, HeI, TiII and FeII. Of special interest is emission in the LiI 6707-A resonance doublet. [OI] and [NII] emission indicate the presence of a nebula around the star. The radial velocity of the absorption lines (AlIII, SiIII, NII and CII) and FeII emission lines agrees with the radial velocity given by Jeffery et al.	en
dc.format.extent	1351746 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/1996MNRAS.282..889P	en
dc.subject	Line:profiles	en
dc.subject	Stars: emission lines	en
dc.subject	BE:stars	en
dc.subject	Stars:individual	en
dc.subject	Mv sgr	en
dc.title	The emission-line spectrum of the hot R Coronae Borealis star MV SGR	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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