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

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dc.creatorChakrabarti, Sandip K.
dc.date1997-03-09
dc.date.accessioned2026-07-07T02:23:03Z
dc.date.available2026-07-07T02:23:03Z
dc.descriptionWe 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.
dc.description13 Latex pages including figures. Macros included. To appear in `Perspective of High Energy Astrophysics', the proceedings of the Golden Jubilee International Colloquium of TIFR (8/96). Eds. P.C. Agarwal et al
dc.identifierhttps://arxiv.org/abs/astro-ph/9703052
dc.identifierhttp://arxiv.org/abs/astro-ph/9703052
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11098
dc.subjectAstrophysics
dc.titleAccretion Processes Around Black Holes And Neutron Stars: Advective Disk Paradigm
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