Radiation Driven Winds from a Self-Similar Slim Disk

Details Radiation Driven Winds from a Self-Similar Slim Disk Radiation Driven Winds from a Self-Similar Slim Disk

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999sf99.proc..280w&link_type=abstract

Star Formation 1999, Proceedings of Star Formation 1999, held in Nagoya, Japan, June 21 - 25, 1999, Editor: T. Nakamoto, Nobeyam

Physics

Scientific paper

We investigated the radiation fields of a self-similar slim disk and the behavior of wind particles, which are driven by the radiation pressure of the disk. When the accretion rate is of the order of a critical rate, the accretion disk becomes Eddington luminosity degree and puff up in the vertical direction to form a so-called slim disk. Our results show clearly that trajectories of wind particles are accelerated along the disk surface. This indicates that the shape of the disk strongly influence the motion of plasma particles. Furthermore, particles lose angular momentum by radiation drag, but gain angular momentum from rotating radiation fields. They tend to spread out in a radial direction.

Affiliated with

Also associated with

No associations

Rating

Radiation Driven Winds from a Self-Similar Slim Disk 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 Radiation Driven Winds from a Self-Similar Slim Disk, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radiation Driven Winds from a Self-Similar Slim Disk will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1061453