Nonlinear Pulsation in the Transonic Region of Geometrically Thin Accretion Disks View Full Text


Ontology type: schema:Chapter     


Chapter Info

DATE

1989

AUTHORS

Ryoji Matsumoto , Shoji Kato , Fumio Honma

ABSTRACT

Nonlinear hydrodynamical simulations are performed to study the evolution of axisymmetric instabilities in viscous accretion disks around a black hole or a nonmagnetized neutron star. When the viscosity parameter α, is sufficiently large (α > 0.05), quasi-periodic pulsations are excited in the innermost transonic region of the disk. Numerical results also show that after the onset of the thermal instability in radiation pressure dominated region, a geometrically thin accretion disk evolves into a slim accretion disk. More... »

PAGES

167-172

Book

TITLE

Theory of Accretion Disks

ISBN

978-94-010-6958-8
978-94-009-1037-9

Author Affiliations

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/978-94-009-1037-9_16

DOI

http://dx.doi.org/10.1007/978-94-009-1037-9_16

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1044634607


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