The reverberation signatures of rotating disc winds in active galactic nuclei

S. W. Mangham, C. Knigge, J. H. Matthews, K. S. Long, S. A. Sim, N. Higginbottom

Research output: Contribution to journalArticle

8 Citations (Scopus)
166 Downloads (Pure)

Abstract

The broad emission lines (BELs) in active galactic nuclei (AGNs) respond to ionizing continuum variations. The time and velocity dependence of their response depends on the structure of the broad-line region: its geometry, kinematics and ionization state. Here, we predict the reverberation signatures of BELs formed in rotating accretion discwinds. We use a Monte Carlo radiative transfer and ionization code to predict velocity-delay maps for representative high- (C iv) and low-ionization (H α) emission lines in both high- and moderate-luminosity AGNs. Self-shielding, multiple scattering and the ionization structure of the outflows are all self-consistently taken into account, while small-scale structure in the outflow is modelled in the microclumping approximation. Our main findings are as follows: (1)The velocity-delay maps of smooth/microclumped outflows often contain significant negative responses. (2) The reverberation signatures of disc-wind models tend to be rotation dominated and can even resemble the classic `red-leads-blue' inflow signature. (3) Traditional`blue-leads-red' outflow signatures can usually only be observed in the long-delay limit. (4) Our models predict lag-luminosity relationships similar to those inferred from observations, but systematically underpredict the observed centroid delays. (5) The ratio between `virial product' and black hole mass predicted by our models depends on viewing angle. Our results imply that considerable care needs to be taken ininterpreting data obtained by observational reverberation mapping campaigns. In particular, basic signatures such as `red-leads-blue',`blue-leads-red' and `blue and red vary jointly' are not always reliable indicators of inflow, outflow or rotation. This may help to explain the perplexing diversity of such signatures seen in observational campaigns to date.
Original languageEnglish
Pages (from-to)4788-4801
Number of pages14
JournalMonthly Notices of the Royal Astronomical Society
Volume471
Issue number4
Early online date22 Jul 2017
DOIs
Publication statusPublished - 11 Nov 2017
Externally publishedYes

Keywords

  • accretion
  • accretion discs
  • radiative transfer
  • quasars: general

Fingerprint Dive into the research topics of 'The reverberation signatures of rotating disc winds in active galactic nuclei'. Together they form a unique fingerprint.

  • Cite this