THE EVENT HORIZON OF M87

The 6 × 10[superscript 9] M[subscript ⊙] supermassive black hole at the center of the giant elliptical galaxy M87 powers a relativistic jet. Observations at millimeter wavelengths with the Event Horizon Telescope have localized the emission from the base of this jet to angular scales comparable to t...

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Main Authors: Broderick, Avery E., Narayan, Ramesh, Kormendy, John, Perlman, Eric S., Rieke, Marcia J., Doeleman, Sheperd Samuel
Other Authors: Haystack Observatory
Format: Article
Language:en_US
Published: IOP Publishing 2015
Online Access:http://hdl.handle.net/1721.1/98485
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author Broderick, Avery E.
Narayan, Ramesh
Kormendy, John
Perlman, Eric S.
Rieke, Marcia J.
Doeleman, Sheperd Samuel
author2 Haystack Observatory
author_facet Haystack Observatory
Broderick, Avery E.
Narayan, Ramesh
Kormendy, John
Perlman, Eric S.
Rieke, Marcia J.
Doeleman, Sheperd Samuel
author_sort Broderick, Avery E.
collection MIT
description The 6 × 10[superscript 9] M[subscript ⊙] supermassive black hole at the center of the giant elliptical galaxy M87 powers a relativistic jet. Observations at millimeter wavelengths with the Event Horizon Telescope have localized the emission from the base of this jet to angular scales comparable to the putative black hole horizon. The jet might be powered directly by an accretion disk or by electromagnetic extraction of the rotational energy of the black hole. However, even the latter mechanism requires a confining thick accretion disk to maintain the required magnetic flux near the black hole. Therefore, regardless of the jet mechanism, the observed jet power in M87 implies a certain minimum mass accretion rate. If the central compact object in M87 were not a black hole but had a surface, this accretion would result in considerable thermal near-infrared and optical emission from the surface. Current flux limits on the nucleus of M87 strongly constrain any such surface emission. This rules out the presence of a surface and thereby provides indirect evidence for an event horizon.
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spelling mit-1721.1/984852022-10-02T00:29:17Z THE EVENT HORIZON OF M87 Broderick, Avery E. Narayan, Ramesh Kormendy, John Perlman, Eric S. Rieke, Marcia J. Doeleman, Sheperd Samuel Haystack Observatory Doeleman, Sheperd Samuel The 6 × 10[superscript 9] M[subscript ⊙] supermassive black hole at the center of the giant elliptical galaxy M87 powers a relativistic jet. Observations at millimeter wavelengths with the Event Horizon Telescope have localized the emission from the base of this jet to angular scales comparable to the putative black hole horizon. The jet might be powered directly by an accretion disk or by electromagnetic extraction of the rotational energy of the black hole. However, even the latter mechanism requires a confining thick accretion disk to maintain the required magnetic flux near the black hole. Therefore, regardless of the jet mechanism, the observed jet power in M87 implies a certain minimum mass accretion rate. If the central compact object in M87 were not a black hole but had a surface, this accretion would result in considerable thermal near-infrared and optical emission from the surface. Current flux limits on the nucleus of M87 strongly constrain any such surface emission. This rules out the presence of a surface and thereby provides indirect evidence for an event horizon. 2015-09-14T18:27:58Z 2015-09-14T18:27:58Z 2015-06 2015-02 Article http://purl.org/eprint/type/JournalArticle 1538-4357 0004-637X http://hdl.handle.net/1721.1/98485 Broderick, Avery E., Ramesh Narayan, John Kormendy, Eric S. Perlman, Marcia J. Rieke, and Sheperd S. Doeleman. “THE EVENT HORIZON OF M87.” The Astrophysical Journal 805, no. 2 (June 2, 2015): 179. © 2015 The American Astronomical Society en_US http://dx.doi.org/10.1088/0004-637x/805/2/179 The Astrophysical Journal Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. application/pdf IOP Publishing IOP Publishing
spellingShingle Broderick, Avery E.
Narayan, Ramesh
Kormendy, John
Perlman, Eric S.
Rieke, Marcia J.
Doeleman, Sheperd Samuel
THE EVENT HORIZON OF M87
title THE EVENT HORIZON OF M87
title_full THE EVENT HORIZON OF M87
title_fullStr THE EVENT HORIZON OF M87
title_full_unstemmed THE EVENT HORIZON OF M87
title_short THE EVENT HORIZON OF M87
title_sort event horizon of m87
url http://hdl.handle.net/1721.1/98485
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