Theoretical constraints on thin disc models for active galactic nuclei

Theoretical constraints on thin disc models for active galactic nuclei

Numerical solutions are presented for the equilibrium structure of a thin disc around a supermassive black hole. The nature and stability of the derived régimes are discussed in the context of accretion disc spectral models for AGN.

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Veröffentlicht in:Monthly notices of the Royal Astronomical Society 1988-12, Vol.235 (3), p.881-894
1. Verfasser: Clarke, Catherine J.
Format: Artikel
Sprache:eng
Schlagworte:
Astronomy
Astrophysics
Earth, ocean, space
Exact sciences and technology
Interstellar medium (ism) and nebulae in external galaxies
Stellar systems. Galactic and extragalactic objects and systems. The universe
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Beschreibung
Zusammenfassung:Numerical solutions are presented for the equilibrium structure of a thin disc around a supermassive black hole. The nature and stability of the derived régimes are discussed in the context of accretion disc spectral models for AGN.
ISSN:0035-8711
1365-2966
DOI:10.1093/mnras/235.3.881