Constraining the geometry of AGN outflows with reflection spectroscopy. (1st June 2018)

• Record Type: Journal Article
• Authors: Parker, M L; Buisson, D J K; Jiang(姜嘉陈), J; Gallo, L C; Kara, E; Matzeu, G A; Walton, D J
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 479:Number 1(2018:Sep.)
• Page Start: L45
• Page End: L49
• Publication Date: 2018-06-01
• Subjects: accretion, accretion discs -- black hole physics -- galaxies: active; Astronomy -- Research -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnrasl/sly096
• Languages: English
• ISSNs: 1745-3933

Abstract

ABSTRACT: We collate active galactic nuclei (AGN) with reported detections of both relativistic reflection and ultrafast outflows. By comparing the inclination of the inner disc from reflection with the line-of-sight velocity of the outflow, we show that it is possible to meaningfully constrain the geometry of the absorbing material. We find a clear relation between the velocity and inclination, and demonstrate that it can potentially be explained either by simple wind geometries or by absorption from the disc surface. Due to systematic errors and a shortage of high-quality simultaneous measurements our conclusions are tentative, but this study represents a proof-of-concept that has a great potential.