Discovery of Pulsations of the B[e] Component in the CI Cam System

Details Discovery of Pulsations of the B[e] Component in the CI Cam System Discovery of Pulsations of the B[e] Component in the CI Cam System

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010vsgh.conf...63b&link_type=abstract

Variable Stars, the Galactic halo and Galaxy Formation, Proceedings of an international conference held in Zvenigorod, Russia, 1

Astronomy and Astrophysics

Astronomy

Scientific paper

We review the studies of rapid variability of the B[e] star CI Cam based on extensive CCD monitoring in two seasons of 2006 and 2008. We found that this variability is caused by pulsations of the B4 III-V component. In the composite frequency spectrum, two pulsation components dominate with periods of 0.416° and 0.266°. In the high resolution BTA/NES spectra taken simultaneously with the photometry, the absorption components in the emission profiles of weak HeI lines temporarily appear. This is typical of pulsating stars.

Affiliated with

Also associated with

No associations

Rating

Discovery of Pulsations of the B[e] Component in the CI Cam System 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 Discovery of Pulsations of the B[e] Component in the CI Cam System, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Discovery of Pulsations of the B[e] Component in the CI Cam System will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1427563