Large-Amplitude Modulations of the Cataclysmic Star ER UMa

Details Large-Amplitude Modulations of the Cataclysmic Star ER UMa Large-Amplitude Modulations of the Cataclysmic Star ER UMa

Sep 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010pobeo..90..147k&link_type=abstract

Publications of the Astronomical Observatory of Belgrade, vol. 90, pp. 147-150

Astronomy and Astrophysics

Astronomy

Scientific paper

We present our BR observations of the cataclysmic star ER UMa covering three consecutive light cycles at quiescence. Their light curves are asymmetric with steeper decreasing branch. While the large light amplitudes of the first two cycles may be expected for the quiescent state, the 0.9^{m} amplitude of the third cycle is unusual big. The period of the observed light modulations in 2008 is shorter than the orbital one. Thus our observations leaded to a discovery of large-amplitude negative superhumps at quiescent state of ER UMa.

Affiliated with

Also associated with

No associations

Rating

Large-Amplitude Modulations of the Cataclysmic Star ER UMa 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 Large-Amplitude Modulations of the Cataclysmic Star ER UMa, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Large-Amplitude Modulations of the Cataclysmic Star ER UMa will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1374578