Astronomy and Astrophysics – Astrophysics
Scientific paper
2003-10-15
Mon.Not.Roy.Astron.Soc. 346 (2003) L21
Astronomy and Astrophysics
Astrophysics
6 pages, 4 figures, to appear in Monthly Notices of the Royal Astronomical Society
Scientific paper
10.1046/j.1365-2966.2003.07290.x
We show that the observed K-velocities and periodicities of AM CVn can be reconciled given a mass ratio of 0.22 and a secondary star with a modest magnetic field of surface strength of order 1 Tesla. We see that the new mass ratio implies that the secondary is most likely semi-degenerate. The effect of the field on the accretion disc structure is examined. The theory of precessing discs and resonant orbits is generalised to encompass higher order resonances than 3:2 and shown to retain consistency with the new mass ratio.
No associations
LandOfFree
Superhumps, Magnetic Fields and the Mass-ratio in AM Canum Venaticorum 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 Superhumps, Magnetic Fields and the Mass-ratio in AM Canum Venaticorum, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Superhumps, Magnetic Fields and the Mass-ratio in AM Canum Venaticorum will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-527165