Abstract
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, the physical conditions in accretion disk coronae remain poorly constrained. Using simultaneous infrared, optical, x-ray, and radio observations of the Galactic black hole system V404 Cygni, showing a rapid synchrotron cooling event in its 2015 outburst, we present a precise 461 ± 12 gauss magnetic field measurement in the corona. This measurement is substantially lower than previous estimates for such systems, providing constraints on physical models of accretion physics in black hole and neutron star binary systems.
Original language | English |
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Pages (from-to) | 1299-1302 |
Number of pages | 4 |
Journal | Science |
Volume | 358 |
Issue number | 6368 |
DOIs | |
Publication status | Published - 8 Dec 2017 |
Externally published | Yes |
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A precise measurement of the magnetic field in the corona of the black hole binary V404 Cygni. / Dallilar, Yigit; Eikenberry, Stephen S.; Garner, Alan; Stelter, Richard D.; Gottlieb, Amy; Gandhi, Poshak; Casella, Piergiorgio; Dhillon, Vik S.; Marsh, Tom R.; Littlefair, Stuart P.; Hardy, Liam; Fender, Rob; Mooley, Kunal; Walton, Dominic J.; Fuerst, Felix; Bachetti, Matteo; Castro-Tirado, A. J.; Charcos, Miguel; Edwards, Michelle L.; Lasso-Cabrera, Nestor M.; Marin-Franch, Antonio; Raines, S. Nicholas; Ackley, Kendall; Bennett, John G.; Cenarro, A. Javier; Chinn, Brian; Donoso, H. Veronica; Frommeyer, Raymond; Hanna, Kevin; Herlevich, Michael D.; Julian, Jeff; Miller, Paola; Mullin, Scott; Murphey, Charles H.; Packham, Chris; Varosi, Frank; Vega, Claudia; Warner, Craig; Ramaprakash, A. N.; Burse, Mahesh; Punnadi, Sujit; Chordia, Pravin; Gerarts, Andreas; De Paz Martín, Héctor; Calero, María Martín; Scarpa, Riccardo; Acosta, Sergio Fernandez; Hernández Sánchez, William Miguel; Siegel, Benjamin; Pérez, Francisco Francisco; Viera Martín, Himar D.; Rodríguez Losada, José A.; Nuñez, Agustín; Tejero, Álvaro; Martín González, Carlos E.; Rodríguez, César Cabrera; Molgó, Jordi; Rodriguez, J. Esteban; Fernández Cáceres, J. Israel; Rodríguez García, Luis A.; Lopez, Manuel Huertas; Dominguez, Raul; Gaggstatter, Tim; Lavers, Antonio Cabrera; Geier, Stefan; Pessev, Peter; Sarajedini, Ata.
In: Science, Vol. 358, No. 6368, 08.12.2017, p. 1299-1302.Research output: Contribution to journal › Article › Research › peer-review
TY - JOUR
T1 - A precise measurement of the magnetic field in the corona of the black hole binary V404 Cygni
AU - Dallilar, Yigit
AU - Eikenberry, Stephen S.
AU - Garner, Alan
AU - Stelter, Richard D.
AU - Gottlieb, Amy
AU - Gandhi, Poshak
AU - Casella, Piergiorgio
AU - Dhillon, Vik S.
AU - Marsh, Tom R.
AU - Littlefair, Stuart P.
AU - Hardy, Liam
AU - Fender, Rob
AU - Mooley, Kunal
AU - Walton, Dominic J.
AU - Fuerst, Felix
AU - Bachetti, Matteo
AU - Castro-Tirado, A. J.
AU - Charcos, Miguel
AU - Edwards, Michelle L.
AU - Lasso-Cabrera, Nestor M.
AU - Marin-Franch, Antonio
AU - Raines, S. Nicholas
AU - Ackley, Kendall
AU - Bennett, John G.
AU - Cenarro, A. Javier
AU - Chinn, Brian
AU - Donoso, H. Veronica
AU - Frommeyer, Raymond
AU - Hanna, Kevin
AU - Herlevich, Michael D.
AU - Julian, Jeff
AU - Miller, Paola
AU - Mullin, Scott
AU - Murphey, Charles H.
AU - Packham, Chris
AU - Varosi, Frank
AU - Vega, Claudia
AU - Warner, Craig
AU - Ramaprakash, A. N.
AU - Burse, Mahesh
AU - Punnadi, Sujit
AU - Chordia, Pravin
AU - Gerarts, Andreas
AU - De Paz Martín, Héctor
AU - Calero, María Martín
AU - Scarpa, Riccardo
AU - Acosta, Sergio Fernandez
AU - Hernández Sánchez, William Miguel
AU - Siegel, Benjamin
AU - Pérez, Francisco Francisco
AU - Viera Martín, Himar D.
AU - Rodríguez Losada, José A.
AU - Nuñez, Agustín
AU - Tejero, Álvaro
AU - Martín González, Carlos E.
AU - Rodríguez, César Cabrera
AU - Molgó, Jordi
AU - Rodriguez, J. Esteban
AU - Fernández Cáceres, J. Israel
AU - Rodríguez García, Luis A.
AU - Lopez, Manuel Huertas
AU - Dominguez, Raul
AU - Gaggstatter, Tim
AU - Lavers, Antonio Cabrera
AU - Geier, Stefan
AU - Pessev, Peter
AU - Sarajedini, Ata
PY - 2017/12/8
Y1 - 2017/12/8
N2 - 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, the physical conditions in accretion disk coronae remain poorly constrained. Using simultaneous infrared, optical, x-ray, and radio observations of the Galactic black hole system V404 Cygni, showing a rapid synchrotron cooling event in its 2015 outburst, we present a precise 461 ± 12 gauss magnetic field measurement in the corona. This measurement is substantially lower than previous estimates for such systems, providing constraints on physical models of accretion physics in black hole and neutron star binary systems.
AB - 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, the physical conditions in accretion disk coronae remain poorly constrained. Using simultaneous infrared, optical, x-ray, and radio observations of the Galactic black hole system V404 Cygni, showing a rapid synchrotron cooling event in its 2015 outburst, we present a precise 461 ± 12 gauss magnetic field measurement in the corona. This measurement is substantially lower than previous estimates for such systems, providing constraints on physical models of accretion physics in black hole and neutron star binary systems.
UR - http://www.scopus.com/inward/record.url?scp=85037639091&partnerID=8YFLogxK
U2 - 10.1126/science.aan0249
DO - 10.1126/science.aan0249
M3 - Article
AN - SCOPUS:85037639091
VL - 358
SP - 1299
EP - 1302
JO - Science
JF - Science
SN - 0036-8075
IS - 6368
ER -