A precise measurement of the magnetic field in the corona of the black hole binary V404 Cygni
Journal
Date Issued
2017
Author(s)
Dallilar, Yigit
•
Eikenberry, Stephen S.
•
Garner, Alan
•
Stelter, Richard D.
•
Gottlieb, Amy
•
Gandhi, Poshak
•
•
Dhillon, Vik S.
•
Marsh, Tom R.
•
Littlefair, Stuart P.
•
Hardy, Liam
•
Fender, Rob
•
Mooley, Kunal
•
Walton, Dominic J.
•
Fuerst, Felix
•
•
Castro-Tirado, A. J.
•
Charcos, Miguel
•
Edwards, Michelle L.
•
Lasso-Cabrera, Nestor M.
•
Marin-Franch, Antonio
•
Raines, S. Nicholas
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Ackley, Kendall
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Bennett, John G.
•
Cenarro, A. Javier
•
Chinn, Brian
•
Donoso, H. Veronica
•
Frommeyer, Raymond
•
Hanna, Kevin
•
Herlevich, Michael D.
•
Julian, Jeff
•
Miller, Paola
•
Mullin, Scott
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Murphey, Charles H.
•
Packham, Chris
•
Varosi, Frank
•
Vega, Claudia
•
Warner, Craig
•
Ramaprakash, A. N.
•
Burse, Mahesh
•
Punnadi, Sujit
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Chordia, Pravin
•
Gerarts, Andreas
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de Paz Martín, Héctor
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Calero, María Martín
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Scarpa, Riccardo
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Acosta, Sergio Fernandez
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Hernández Sánchez, William Miguel
•
Siegel, Benjamin
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Pérez, Francisco Francisco
•
Viera Martín, Himar D.
•
Rodríguez Losada, José A.
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Nuñez, Agustín
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Tejero, Álvaro
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Martín González, Carlos E.
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Rodríguez, César Cabrera
•
Molgó, Jordi
•
Rodriguez, J. Esteban
•
Cáceres, J. Israel Fernández
•
Rodríguez García, Luis A.
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Lopez, Manuel Huertas
•
Dominguez, Raul
•
Gaggstatter, Tim
•
Lavers, Antonio Cabrera
•
Geier, Stefan
•
Pessev, Peter
•
Sarajedini, Ata
Abstract
The binary system V404 Cygni consists of a red giant star orbiting a black hole. In 2015, a surge of accretion by the black hole caused the surrounding plasma to brighten suddenly for the first time since 1989, briefly becoming the brightest x-ray source in the sky. Dallilar et al. combined observations from radio, infrared, optical, and x-ray telescopes taken during the outburst. They compared how fast the flux decayed at each wavelength, which allowed them to constrain the size of the emitting region, determine that the plasma within it cooled through synchrotron radiation, and measure the magnetic field around the black hole.
Volume
358
Issue
6368
Start page
1299
Issn Identifier
0036-8075
Ads BibCode
2017Sci...358.1299D
Rights
restricted
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