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.

Citation

(2007). Disc-Magnetosphere interactions in Cataclysmic Variable Stars. Proceedings of the International Astronomical Union, https://doi.org/10.1017/S1743921307009684

• Publication Date: Dec 15, 2007
• Journal: Proceedings of the International Astronomical Union
• Print ISSN: 1743-9213
• Publisher: Cambridge University Press
• DOI: https://doi.org/10.1017/S1743921307009684
• Keywords: astrophysics, accretion, accretion disks, magnetic fields, binaries, close, novae, cataclysmic variables, X-rays, stars
• Publisher URL: http://dx.doi.org/10.1017/S1743921307009684