Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2814
Title: The emission-line spectrum of the hot R Coronae Borealis star MV SGR
Authors: Pandey, G
Kameswara Rao, N
Lambert, D. L
Keywords: Line:profiles;Stars: emission lines;BE:stars;Stars:individual;Mv sgr
Issue Date: Oct-1996
Publisher: Royal Astronomical Society
Citation: Monthly Notices of the Royal Astronomical Society, Vol. 282, No. 3, pp. 889 - 899
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.
URI: http://hdl.handle.net/2248/2814
ISSN: 0035-8711
???metadata.dc.relation.uri???: http://adsabs.harvard.edu/abs/1996MNRAS.282..889P
Appears in Collections:IIAP Publications

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