Powerful Flares From Recoiling Black Holes In Quasars
dc.contributor.utaustinauthor | Shields, Gregory A. | en_US |
dc.contributor.utaustinauthor | Bonning, E. W. | en_US |
dc.creator | Shields, Gregory A. | en_US |
dc.creator | Bonning, E. W. | en_US |
dc.date.accessioned | 2016-04-28T19:33:29Z | |
dc.date.available | 2016-04-28T19:33:29Z | |
dc.date.issued | 2008-08 | en |
dc.description.abstract | Mergers of spinning black holes can give recoil velocities from gravitational radiation up to several thousand km s(-1). A recoiling supermassive black hole in an AGN retains the inner part of its accretion disk. Marginally bound material rejoining the disk around the moving black hole releases a large amount of energy in shocks in a short time, leading to a flare in thermal soft X-rays with a luminosity approaching the Eddington limit. Reprocessing of the X-rays by the infalling material gives strong optical and ultraviolet emission lines with a distinctive spectrum. Despite the short lifetime of the flare (similar to 10(4) yr), as many as 10(2) flares may be in play at the present time in QSOs at redshifts similar to 1-3. These flares provide a means to identify high-velocity recoils. | en_US |
dc.description.department | Astronomy | en_US |
dc.description.sponsorship | European Fellowship MIF1-CT-2005-008762 | en_US |
dc.identifier | doi:10.15781/T22Z3G | |
dc.identifier.Filename | 2008_08_powerfulflares.pdf | en_US |
dc.identifier.citation | Shields, Gregory A., and E. W. Bonning. "Powerful flares from recoiling black holes in quasars." The Astrophysical Journal, Vol. 682, No. 2 (Aug., 2008): 758. | en_US |
dc.identifier.doi | 10.1086/589427 | en_US |
dc.identifier.issn | 0004-637X | en_US |
dc.identifier.uri | http://hdl.handle.net/2152/34733 | |
dc.language.iso | English | en_US |
dc.relation.ispartof | en_US | |
dc.relation.ispartofserial | Astrophysical Journal | en_US |
dc.rights | Administrative deposit of works to Texas ScholarWorks: This works author(s) is or was a University faculty member, student or staff member; this article is already available through open access or the publisher allows a PDF version of the article to be freely posted online. The library makes the deposit as a matter of fair use (for scholarly, educational, and research purposes), and to preserve the work and further secure public access to the works of the University. | en_US |
dc.rights.restriction | Open | en_US |
dc.subject | black hole physics | en_US |
dc.subject | galaxies : active | en_US |
dc.subject | quasars : general | en_US |
dc.subject | digital sky survey | en_US |
dc.subject | active galactic nuclei | en_US |
dc.subject | gravitational-radiation | en_US |
dc.subject | binaries | en_US |
dc.subject | coalescence | en_US |
dc.subject | spectra | en_US |
dc.subject | agn | en_US |
dc.subject | astronomy & astrophysics | en_US |
dc.title | Powerful Flares From Recoiling Black Holes In Quasars | en_US |
dc.type | Article | en_US |