On BLR Size Estimates in Reverberation Models
Abstract
Following the approach of Melnikov & Shevchenko (2008), we explore how the nonlinearity in the emission-line luminosity Ll of a broad-line region cloud, in its dependence on the ionizing continuum flux Fi incident on the cloud, affects estimates of the size of the broad-line region by means of cross-correlation methods. We show that the estimates obtained by straightforward cross-correlation of emission-line and continuum light curves can significantly underestimate the BLR size. We demonstrate examples of direct reverberation modelling of AGN emission-line light curves taking into account the nonlinearity of the “Ll-Fi” relation. This nonlinearity allows one to explain the differences in the time lags for different lines. Cross-correlation estimates of the BLR size turn out to be small in comparison to the estimates obtained by the direct reverberation modelling.
- Publication:
-
Co-Evolution of Central Black Holes and Galaxies
- Pub Date:
- May 2010
- DOI:
- 10.1017/S1743921310006290
- Bibcode:
- 2010IAUS..267..209M
- Keywords:
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- galaxies: nuclei;
- galaxies: Seyfert;
- quasars: emission lines