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Ram-pressure Stripping of a Kicked Hill Sphere: Prompt Electromagnetic Emission from the Merger of Stellar Mass Black Holes in an AGN Accretion Disk

McKernan, B. and Ford, K. E. S. and Bartos, I. and Graham, M. J. and Lyra, W. and Márka, S. and Márka, Z. and Ross, N. P. and Stern, D. and Yang, Y. (2019) Ram-pressure Stripping of a Kicked Hill Sphere: Prompt Electromagnetic Emission from the Merger of Stellar Mass Black Holes in an AGN Accretion Disk. Astrophysical Journal Letters, 884 (2). Art. No. L50. ISSN 2041-8213. https://resolver.caltech.edu/CaltechAUTHORS:20191023-090812298

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Abstract

Accretion disks around supermassive black holes (SMBHs) are promising sites for stellar mass black hole (BH) mergers due to mass segregation and merger acceleration by disk gas torques. Here we show that a gravitational-wave (GW) kick at BH merger causes ram-pressure stripping of gas within the BH Hill sphere. If R_H ≥ H, the disk height, an off-center UV flare at a_(BH) ~ 10³ r_g, emerges within t_(UV) ~ O(2 days)(a_(BH)/10³ r_g)(M_(SMBH)/10⁸ M_⊙)(v_(kick)/10² km s⁻¹) postmerger and lasts O(R_H/v_(kick)) ~ O(5t_(UV)). The flare emerges with luminosity O(10⁴² erg s⁻¹(t_(UV)/2 days)⁻¹(M_(Hill)/1M_⊙)(v_(kick)/10² km s⁻¹)². Active galactic nucleus optical/UV photometry is altered and asymmetric broad emission line profiles can develop after weeks. If R_H < H, detectability depends on disk optical depth. Follow-up by large optical sky surveys is optimized for small GW error volumes and for Laser Interferometer Gravitational-Wave Observatory/Virgo triggers >50M_⊙.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.3847/2041-8213/ab4886DOIArticle
https://arxiv.org/abs/1907.03746arXivDiscussion Paper
ORCID:
AuthorORCID
McKernan, B.0000-0002-9726-0508
Bartos, I.0000-0001-5607-3637
Graham, M. J.0000-0002-3168-0139
Lyra, W.0000-0002-3768-7542
Ross, N. P.0000-0003-1830-6473
Stern, D.0000-0003-2686-9241
Additional Information:© 2019 The American Astronomical Society. Received 2019 July 5; revised 2019 September 8; accepted 2019 September 27; published 2019 October 17. B.M. dedicates this paper to the memory of his mother, Treasa McKernan. B.M. and K.E.S.F. are supported by NSF 1831412. The work of D.S. was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with NASA. Thanks to the referee for highlighting the GW kick and participants in the 1st workshop on stellar mass BH mergers in AGN disks, held 2019 March 11–13, and sponsored by the CCA at the Flatiron Institute in New York City.
Funders:
Funding AgencyGrant Number
NSFAST-1831412
NASA/JPL/CaltechUNSPECIFIED
Subject Keywords:Black holes; Active galactic nuclei; Gravitational waves; Gravitational wave astronomy
Issue or Number:2
Classification Code:Unified Astronomy Thesaurus concepts: Black holes (162); Active galactic nuclei (16); Gravitational waves (678); Gravitational wave astronomy (675)
Record Number:CaltechAUTHORS:20191023-090812298
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20191023-090812298
Official Citation:B. McKernan et al 2019 ApJL 884 L50
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:99404
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:23 Oct 2019 16:49
Last Modified:09 Mar 2020 13:19

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