Broadband spectral energy distribution of active galactic nuclei

Details Broadband spectral energy distribution of active galactic nuclei Broadband spectral energy distribution of active galactic nuclei

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004asthe..97..694k&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 97, No. 12, p. 694 - 705 (2004)

Astronomy and Astrophysics

Astronomy

1

Active Galactic Nuclei, Spectral Energy Distribution

Scientific paper

The central engine of an active galactic nucleus (AGN) is as small as the solar system, while it often outshines its host galaxy. We have explored some theoretical aspects of the broadband spectral energy distribution of AGNs, aiming at revealing their physical condition, radiative processes, formation and growth. Here, our recent findings regarding on sub-Eddington and super-Eddington accreting AGNs are briefly summarized, together with some results obtained through our XMM-Newton observation.

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