We constrain the intrinsic Eddington ratio (LambdaEdd) distribution function for local active galactic nuclei (AGN) in bins of low and high obscuration [log(NH/cm−2)<=22and 22-1, the trend is reversed, with <30% of AGN having log(NH/cm−2)>22, which we suggest is mainly due to the small fraction of time spent in a highly obscured state. Considering the Eddington ratio distribution function of narrow-line and broad-line AGN from our prior work, we see a qualitatively similar picture. To disentangle temporal and geometric effects at high LambdaEdd, we explore plausible clearing scenarios such that the time-weighted covering factors agree with the observed population ratio. We find that the low fraction of obscured AGN at high LambdaEdd is primarily due to the fact that the covering factor drops very rapidly, with more than half the time spent with <10% covering factor. We also find that nearly all obscured AGN at high-LambdaEdd exhibit some broad lines. We suggest that this is because the height of the depleted torus falls below the height of the broad-line region, making the latter visible from all lines of sight.
Ananna T.T., Urry C.M., Ricci C., Natarajan P., Hickox R.C., Trakhtenbrot B., et al. (2022). Probing the Structure and Evolution of BASS Active Galactic Nuclei through Eddington Ratios. THE ASTROPHYSICAL JOURNAL LETTERS, 939(1), 1-8 [10.3847/2041-8213/ac9979].
Probing the Structure and Evolution of BASS Active Galactic Nuclei through Eddington Ratios
Marchesi S.Writing – Review & Editing
;
2022
Abstract
We constrain the intrinsic Eddington ratio (LambdaEdd) distribution function for local active galactic nuclei (AGN) in bins of low and high obscuration [log(NH/cm−2)<=22and 22-1, the trend is reversed, with <30% of AGN having log(NH/cm−2)>22, which we suggest is mainly due to the small fraction of time spent in a highly obscured state. Considering the Eddington ratio distribution function of narrow-line and broad-line AGN from our prior work, we see a qualitatively similar picture. To disentangle temporal and geometric effects at high LambdaEdd, we explore plausible clearing scenarios such that the time-weighted covering factors agree with the observed population ratio. We find that the low fraction of obscured AGN at high LambdaEdd is primarily due to the fact that the covering factor drops very rapidly, with more than half the time spent with <10% covering factor. We also find that nearly all obscured AGN at high-LambdaEdd exhibit some broad lines. We suggest that this is because the height of the depleted torus falls below the height of the broad-line region, making the latter visible from all lines of sight.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
