Accretion Discs Trapped Near Corotation

Details Accretion Discs Trapped Near Corotation Accretion Discs Trapped Near Corotation

2011-08-18

arxiv.org/abs/1108.3833v2

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

14 pages, 10 figures, accepted to MNRAS

Scientific paper

We show that discs accreting onto the magnetosphere of a rotating star can end up in a 'trapped' state, in which the inner edge of the disc stays near the corotation radius, even at low and varying accretion rates. The accretion in these trapped states can be steady or cyclic; we explore these states over wide range of parameter space. We find two distinct regions of instability, one related to the buildup and release of mass in the disk outside corotation, the other to mass storage within the transition region near corotation. With a set of calculations over long time scales we show how trapped states evolve from both nonaccreting and fully accreting initial conditions, and also calculate the effects of cyclic accretion on the spin evolution of the star. Observations of cycles such as found here would provide important clues on the physics of magnetospheric accretion. Recent observations of cyclic and other unusual variability in T Tauri stars (EXors) and X-ray binaries are discussed in this context.

Affiliated with

Also associated with

No associations

Rating

Accretion Discs Trapped Near Corotation 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 Accretion Discs Trapped Near Corotation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Accretion Discs Trapped Near Corotation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-107538