Powerful Flares From Recoiling Black Holes In Quasars

dc.contributor.utaustinauthorShields, Gregory A.en_US
dc.contributor.utaustinauthorBonning, E. W.en_US
dc.creatorShields, Gregory A.en_US
dc.creatorBonning, E. W.en_US
dc.date.accessioned2016-04-28T19:33:29Z
dc.date.available2016-04-28T19:33:29Z
dc.date.issued2008-08en
dc.description.abstractMergers 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.departmentAstronomyen_US
dc.description.sponsorshipEuropean Fellowship MIF1-CT-2005-008762en_US
dc.identifierdoi:10.15781/T22Z3G
dc.identifier.Filename2008_08_powerfulflares.pdfen_US
dc.identifier.citationShields, 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.doi10.1086/589427en_US
dc.identifier.issn0004-637Xen_US
dc.identifier.urihttp://hdl.handle.net/2152/34733
dc.language.isoEnglishen_US
dc.relation.ispartofen_US
dc.relation.ispartofserialAstrophysical Journalen_US
dc.rightsAdministrative 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.restrictionOpenen_US
dc.subjectblack hole physicsen_US
dc.subjectgalaxies : activeen_US
dc.subjectquasars : generalen_US
dc.subjectdigital sky surveyen_US
dc.subjectactive galactic nucleien_US
dc.subjectgravitational-radiationen_US
dc.subjectbinariesen_US
dc.subjectcoalescenceen_US
dc.subjectspectraen_US
dc.subjectagnen_US
dc.subjectastronomy & astrophysicsen_US
dc.titlePowerful Flares From Recoiling Black Holes In Quasarsen_US
dc.typeArticleen_US

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