Accretion Processes Around Black Holes And Neutron Stars: Advective Disk Paradigm

Details Accretion Processes Around Black Holes And Neutron Stars: Advective Disk Paradigm Accretion Processes Around Black Holes And Neutron Stars: Advective Disk Paradigm

1997-03-09

arxiv.org/abs/astro-ph/9703052v1

Astronomy and Astrophysics

Astrophysics

13 Latex pages including figures. Macros included. To appear in `Perspective of High Energy Astrophysics', the proceedings of

Scientific paper

We review models which include advective accretion disks onto compact objects and discuss the influence of the centrifugal pressure supported high density region close to the compact objects on the emitted spectra. We show that the stationary and non-stationary spectral properties (such as low and high states, quasi-periodic oscillations, quiescent and rising phases of X-ray novae, etc.) of black hole candidates could be satisfactorily explained by the advective disk models.

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