Emission Spectrum of Hot R CrB star Mv Sgr

dc.contributor.author	Kameswara Rao, N
dc.contributor.author	Houziaux, L
dc.contributor.author	Giridhar, S
dc.date.accessioned	2008-09-17T11:52:56Z
dc.date.available	2008-09-17T11:52:56Z
dc.date.issued	1990-03
dc.identifier.citation	Journal of Astrophysics and Astronomy, Vol.11, No. 1, pp. 37 - 42	en
dc.identifier.issn	0250-6335
dc.identifier.uri	http://hdl.handle.net/2248/3708
dc.description.abstract	The new spectroscopic observation of MV Sgr obtained at ESO in 1987july shows enhanced emission lines of He I , λ 3889, [S II ] λ 4068 relative to the observations discussed by Jeffrey et al. (1988). The presence of [SII] λ 4068 indicates the presence of planetary nebulae like envelope around the star. Although the radial velocity of the absorption lines and Fe II emission lines do agree with the velocity given by Jeffery et. al., the [S II] λ 4068 and probably He I emission lines appear to behave differently	en
dc.language.iso	en	en
dc.publisher	Indian Academy Sciences	en
dc.relation.uri	http://ads.iucaa.ernet.in/abs/1990JApA...11...37R	en
dc.subject	Stars	en
dc.subject	R Cr B type – stars	en
dc.subject	Nebulosites- stars	en
dc.subject	Individual	en
dc.title	Emission Spectrum of Hot R CrB star Mv Sgr	en
dc.type	Article	en