Long-term Spectroscopic Variability of Two Oe Stars

Details Long-term Spectroscopic Variability of Two Oe Stars Long-term Spectroscopic Variability of Two Oe Stars

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ibvs.5773....1r&link_type=abstract

Information Bulletin on Variable Stars, 5773, 1.

Physics

6

Star: Spectroscopy, - Stars: Early-Type, - Stars: Variables

Scientific paper

HD 45314 and HD 60848 are poorly studied Oe-type stars. Spectroscopic
monitoring over 5 years reveals strong variations in the strength of the
emission lines and for HD 45314 in the V/R ratio of the double-peaked
emissions. Part of these long-term variations could be recurrent.

Affiliated with

Also associated with

No associations

Rating

Long-term Spectroscopic Variability of Two Oe Stars 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 Long-term Spectroscopic Variability of Two Oe Stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Long-term Spectroscopic Variability of Two Oe Stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-770347