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Emission spectrum of hot R OB star MV Sgr
Authors:N Kameswara Rao  L Houziaux  Sunetra Giridhar
Institution:(1) Indian Institute of Astrophysics, 560034 Bangalore;(2) Instut d’ Astrophysique, Universite de Liège, Liege, Belgium;(3) Indian Institute of Astrophysics, 560034 Bangalore
Abstract:The new spectroscopic observation of MV Sgr obtained at ESO in 1987 July shows enhanced emission lines of He I λ3889, SII] λ4068 relative to the observations discussed by Jeffreyet al. (1988). The presence of SII] λ4068 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 Jeffreyet al., the SII] λ4068 and probably He I emission lines appear to behave differently. Based on observations collected at the European Southern Observatory, La Silla, Chile.
Keywords:stars  R CrB type  stars  nebulosities  stars  individual
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