The Structure of the Broad-Line Region in Well-Studied AGNs

Details The Structure of the Broad-Line Region in Well-Studied AGNs The Structure of the Broad-Line Region in Well-Studied AGNs

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997osu..rept.....p&link_type=abstract

Technical Report, Ohio State Univ. Columbus, OH United States

Computer Science

Active Galactic Nuclei, Photoionization, Light Emission, Ultraviolet Emission, Transfer Functions, Computer Programs

Scientific paper

Large amounts of high quality UV and optical data have been obtained in massive multi-wavelength monitoring campaigns on a small number of active galactic nuclei, and these data are changing our understanding of the central engines in these sources in a fundamental way. Preliminary analyses have shown that more comprehensive approaches will be necessary to make full use of these data. We propose to undertake a complete set of photoionization equilibrium calculations with a state-of-the-art computer code in order to determine the radial structure of the broad-line region in a way that is consistent with the emission-line fluxes, profiles, and transfer functions.

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