V1500 Cyg: 25 years later

Details V1500 Cyg: 25 years later V1500 Cyg: 25 years later

Jan 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aspc..261..651p&link_type=abstract

The Physics of Cataclysmic Variables and Related Objects, ASP Conference Proceedings, Vol. 261. Edited by B. T. Gänsicke, K. Beu

Physics

2

Scientific paper

We present photometry of the asynchronous polar Nova Cygni 1975 = V1500 Cyg in a 25 years after its outburst. This binary clearly shows light variations both at the orbital period, and at the spin-orbital beat period, 8.4 d, which indicates asynchronous motion of the binary components. The orbital R amplitudes are practically constant over the beat period. This could be caused by the variable accretion rate/brightness of a ring surrounding the white dwarf depending on the orientation of the white dwarf magnetic pole in respect to the red dwarf.

Affiliated with

Also associated with

No associations

Rating

V1500 Cyg: 25 years later 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 V1500 Cyg: 25 years later, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and V1500 Cyg: 25 years later will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1087753