Density and Ionization Parameters of Line and Continuum Emission from the Outer Regions of Accretion Disk in Active Galactic Nuclei

Details Density and Ionization Parameters of Line and Continuum Emission from the Outer Regions of Accretion Disk in Active Galactic Nuclei Density and Ionization Parameters of Line and Continuum Emission from the Outer Regions of Accretion Disk in Active Galactic Nuclei

Oct 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998chphl..15..778l&link_type=abstract

Chinese Physics Letters, Volume 15, Issue 10, pp. 778-780 (1998).

Physics

3

Scientific paper

In this paper, the diffusion source model and the structure of magnetized accretion disk with self-gravity are used to study the density and the ionization parameter of the HII and HI* zone, of which most likely the broad line emitting region consists. Two different densities and ionization parameters are determined: the first langlen(HII)rangle and Ξ(HII), corresponding to the mean density and ionization parameter in the completely ionized HII zone, and the second, langlen(HI*)rangle and Ξ(HI*), to the mean density and ionization parameters in the HI* zone.

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