Disc magnetosphere interactions in cataclysmic variable stars
Abstract
I review, from an observational perspective, the interactions of accretion discs with magnetic fields in cataclysmic variable stars. I start with systems where the accretion flows via a stream, and discuss the circumstances in which the stream forms into an accretion disc, pointing to stars which are close to this transition. I then turn to disc-fed systems and discuss what we know about how material threads on to field lines, as deduced from the pattern of accretion footprints on the white dwarf. I discuss whether distortions of the field lines are related to accretion torques and the changing spin periods of the white dwarfs. I also review the effect on the disc-magnetosphere interaction of disc-instability outbursts. Lastly, I discuss the temporary, dynamo-driven magnetospheres thought to occur in dwarf-nova outbursts, and whether slow-moving waves are excited at the inner edges of the disc.
- Publication:
-
Star-Disk Interaction in Young Stars
- Pub Date:
- May 2007
- DOI:
- 10.1017/S1743921307009684
- arXiv:
- arXiv:0712.2520
- Bibcode:
- 2007IAUS..243..325H
- Keywords:
-
- Accretion;
- accretion disks;
- magnetic fields;
- binaries: close;
- novae;
- cataclysmic variables;
- X-rays: stars;
- Astrophysics
- E-Print:
- Invited review at IAU Symp. 243 (12 pages)