The development of large-scale instability in stellar accretion disks and its influence on the redistribution of angular momentum

Details The development of large-scale instability in stellar accretion disks and its influence on the redistribution of angular momentum The development of large-scale instability in stellar accretion disks and its influence on the redistribution of angular momentum

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008arep...52..811l&link_type=abstract

Astronomy Reports, Volume 52, Issue 10, pp.811-814

Astronomy and Astrophysics

Astronomy

1

97.10.Gz, 95.30.Lz

Scientific paper

The paper continues our studies of large-scale instability arising during shearmotions in stellar accretion disks due to the development of small perturbations. The evolution of a local perturbation introduced into the outer part of a stationary accretion disk is modeled mathematically. The possible formation of large-scale structures that propagate throughout the disk, leading to an appreciable redistribution of angular momentum, is demonstrated.

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