Theoretical constraints on thin disc models for active galactic nuclei

Details Theoretical constraints on thin disc models for active galactic nuclei Theoretical constraints on thin disc models for active galactic nuclei

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988mnras.235..881c&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 235, Dec. 15, 1988, p. 881-894.

Statistics

Computation

30

Accretion Disks, Active Galactic Nuclei, Black Holes (Astronomy), Computational Astrophysics, Equilibrium Equations, Galactic Structure, Numerical Stability

Scientific paper

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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