A precise measurement of the magnetic field in the corona of the black hole binary V404 Cygni

Observations of binary stars containing an accreting black hole or neutron star often show x-ray emission extending to high energies (>10 kilo--electron volts), which is ascribed to an accretion disk corona of energetic particles akin to those seen in the solar corona. Despite their ubiquity,...

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Bibliographic Details
Main Authors:	Dallilar, Y, Eikenberry, SS, Garner, A, Stelter, RD, Gottlieb, A, Gandhi, P, Casella, P, Dhillon, VS, Marsh, TR, Littlefair, SP, Hardy, L, Fender, R, Mooley, K, Walton, DJ, Fuerst, F, Bachetti, M, Castro-Tirado, AJ, Charcos, M, Edwards, ML, Lasso-Cabrera, NM, Marin-Franch, A, Raines, SN, Ackley, K, Bennett, JG, Cenarro, AJ, Chinn, B, Donoso, HV, Frommeyer, R, Hanna, K, Herlevich, MD, Julian, J, Miller, P, Mullin, S, Murphey, CH, Packham, C, Varosi, F, Vega, C, Warner, C, Ramaprakash, AN, Burse, M, Punnadi, S, Chordia, P, Gerarts, A, De Paz Martín, H, Calero, MM, Scarpa, R, Acosta, SF, Sánchez, WM, Siegel, B, Pérez, FF, Martín, HD, Losada, JA, Nuñez, A, Tejero, Á, González, CE, Rodríguez, CC, Molgó, J, Rodriguez, JE, Cáceres, JIF, LA Rodríguez García, Lopez, MH, Dominguez, R, Gaggstatter, T, Lavers, AC, Geier, S, Pessev, P, Sarajedini, A
Format:	Journal article
Language:	English
Published:	American Association for the Advancement of Science 2017

A precise measurement of the magnetic field in the corona of the black hole binary V404 Cygni

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