Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992mnras.258..189r&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 258, no. 1, Sept. 1, 1992, p. 189-197. Research support
Astronomy and Astrophysics
Astronomy
156
Accretion Disks, Active Galactic Nuclei, Emission Spectra, X Ray Astronomy, Black Holes (Astronomy), Compton Effect, X Ray Spectra
Scientific paper
We present fully self-consistent calculations of the spectra emitted by accretion disks in active galactic nuclei. We treat the inner, radiation-pressure-dominated regions of standard alpha-disks. Incoherent Compton scattering and emission/absorption of radiation by hydrogen and helium are included in compting the vertical temperature structure within the disk and the emergent spectrum. Comptonization modifies the EUV/soft X-ray continuum and the He II spectral features. In particular, an important fraction of the emergent luminosity appears in the form of a steep soft X-ray spectrum. The observed UV flux and soft X-ray excess of Mkn 841 are consistent with a face-on accretion disk with alpha = 0.1 surrounding a black hole.
Fabian Andrea C.
Mineshige Shin
Ross Ronald R.
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