Astronomy and Astrophysics – Astronomy
Scientific paper
May 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21642001s&link_type=abstract
American Astronomical Society, AAS Meeting #216, #420.01; Bulletin of the American Astronomical Society, Vol. 41, p.831
Astronomy and Astrophysics
Astronomy
Scientific paper
We compare QSO emission-line spectra to predictions based on theoretical ionizing continua of accretion disks. The observed line intensities do not show the expected trend of higher ionization with higher accretion disk temperature. This suggests that, at least for accretion rates close to the Eddington limit, the inner disk does not reach temperatures as high as expected from standard disk theory. Modified radial temperature profiles, including some models previously proposed in the literature, achieve better agreement with observation.
Bonning Erin Wells
Shields Gregory A.
Smith Kermit L.
Stevens Alyx
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