Physics
Scientific paper
May 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..370..225b&link_type=abstract
Solar and Stellar Physics Through Eclipses ASP Conference Series, Vol. 370, proceedings of the conference held 27-29 March, 2006
Physics
3
Scientific paper
We present new UBV photometric observations obtained in the last four observing seasons and one season of spectroscopic observation for the Be star EM Cep. A possible period of 0.403 days and large light amplitude variations from one season to other were determined from the new photometric observations. A flare activity for this star has been detected on 17-18 July 2003. The brightness increase during the flare was found to be maximum in U-band. New spectroscopic observations with high-resolution spectrograph did not present a certain result due to the limited number of data. The type of variability in the light curves shows that the star could be a λ Eri-type variable. Additional changes on the light curve do not show any periodicity. Binarity problem of the star has been also discussed.
Bakis Hicran
Bakis Volkan
Budding Edwin
Demircan Osman
Tanriver Mehmet
No associations
LandOfFree
On the Light Curve Variation of the Be Star EM Cep 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 On the Light Curve Variation of the Be Star EM Cep, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the Light Curve Variation of the Be Star EM Cep will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-765538