dc.contributor.author |
Pandey, G |
|
dc.contributor.author |
Kameswara Rao, N |
|
dc.contributor.author |
Lambert, D. L |
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dc.date.accessioned |
2008-07-22T11:35:42Z |
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dc.date.available |
2008-07-22T11:35:42Z |
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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 |
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dc.identifier.uri |
http://hdl.handle.net/2248/2814 |
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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. |
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dc.format.extent |
1351746 bytes |
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dc.format.mimetype |
application/pdf |
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dc.language.iso |
en |
en |
dc.publisher |
Royal Astronomical Society |
en |
dc.relation.uri |
http://adsabs.harvard.edu/abs/1996MNRAS.282..889P |
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dc.subject |
Line:profiles |
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dc.subject |
Stars: emission lines |
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dc.subject |
BE:stars |
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dc.subject |
Stars:individual |
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dc.subject |
Mv sgr |
en |
dc.title |
The emission-line spectrum of the hot R Coronae Borealis star MV SGR |
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dc.type |
Article |
en |