Runaway instability in accretion disks orbiting black holes
- 1 April 1983
- journal article
- Published by Springer Nature in Nature
- Vol. 302 (5909) , 597-599
- https://doi.org/10.1038/302597a0
Abstract
No abstract availableKeywords
This publication has 13 references indexed in Scilit:
- Physical properties of thick supercritical accretion disksThe Astrophysical Journal, 1982
- Ion-supported tori and the origin of radio jetsNature, 1982
- Recurrent Seyfert activity in spiral galaxy nucleiNature, 1981
- Innermost parts of accretion disks are thermally and secularly stableNature, 1981
- Rotation-induced bistability of transonic accretion onto a black holeThe Astrophysical Journal, 1981
- Thick accretion disks with super-Eddington luminositiesThe Astrophysical Journal, 1980
- Perturbation of a slowly rotating black hole by a stationary axisymmetric ring of matter. II - Penrose processes, circular orbits, and differential mass formulaeThe Astrophysical Journal, 1975
- Perturbation of a Slowly Rotating Black Hole by a Stationary Axisymmetric Ring of Matter. I. Equilibrium ConfigurationsThe Astrophysical Journal, 1974
- The Equilibrium of Self-Gravitating Rings.The Astrophysical Journal, 1964
- Evolutionaty Mass Exchange in Close Binary Systems.The Astrophysical Journal, 1960