The 2003 Superoutburst of an SU UMa-Type Dwarf Nova, GO Comae Berenicis

Details The 2003 Superoutburst of an SU UMa-Type Dwarf Nova, GO Comae Berenicis The 2003 Superoutburst of an SU UMa-Type Dwarf Nova, GO Comae Berenicis

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005pasj...57..193i&link_type=abstract

Publications of the Astronomical Society of Japan, Vol.57, No.1, pp. 193-201

Astronomy and Astrophysics

Astronomy

16

Accretion, Accretion Disks, Stars: Dwarf Novae, Stars: Individual (Go Comae Berenicis), Stars: Novae, Cataclysmic Variables, Stars: Oscillations

Scientific paper

We photometrically observed a 2003 June superoutburst of GO Gom. The mean superhump period was 0.063059(13)d. The resultant data revealed that (1) the obtained light curve contained a precursor, (2) a plateau stage of the object lasted for 8 days, which is remarkably shorter than that of ordinary SU UMa-type dwarf novae, and (3) the amplitude of the superoutburst was less than 5mag, which is unpredictably small when taking into account the fact that the supercycle of GO Com is about 2800 days. In order to explain these anomalies, a mass-elimination process from the accretion disk, such as evaporation, may play an important role.

Affiliated with

Also associated with

No associations

Rating

The 2003 Superoutburst of an SU UMa-Type Dwarf Nova, GO Comae Berenicis 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 2003 Superoutburst of an SU UMa-Type Dwarf Nova, GO Comae Berenicis, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The 2003 Superoutburst of an SU UMa-Type Dwarf Nova, GO Comae Berenicis will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-823767