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

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

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996mnras.282..889p&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 282, Issue 3, pp. 889-899.

Astronomy and Astrophysics

Astronomy

5

Line: Profiles, Stars: Emission-Line, Be, Stars: Individual: Mv Sgr

Scientific paper

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.

Affiliated with

Also associated with

No associations

Rating

The emission-line spectrum of the hot R Coronae Borealis star MV SGR does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The emission-line spectrum of the hot R Coronae Borealis star MV SGR, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The emission-line spectrum of the hot R Coronae Borealis star MV SGR will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1137601