The response of relativistic outflowing gas to the inner accretion disk of a black hole

Michael L. Parker (), Ciro Pinto, Andrew C. Fabian, Anne Lohfink, Douglas J. K. Buisson, William N. Alston, Erin Kara, Edward M. Cackett, Chia-Ying Chiang, Thomas Dauser, Barbara De Marco, Luigi C. Gallo, Javier Garcia, Fiona A. Harrison, Ashley L. King, Matthew J. Middleton, Jon M. Miller, Giovanni Miniutti, Christopher S. Reynolds, Phil Uttley, Ranjan Vasudevan, Dominic J. Walton, Daniel R. Wilkins and Abderahmen Zoghbi
Additional contact information
Michael L. Parker: Institute of Astronomy
Ciro Pinto: Institute of Astronomy
Andrew C. Fabian: Institute of Astronomy
Anne Lohfink: Institute of Astronomy
Douglas J. K. Buisson: Institute of Astronomy
William N. Alston: Institute of Astronomy
Erin Kara: University of Maryland
Edward M. Cackett: Wayne State University
Chia-Ying Chiang: Wayne State University
Thomas Dauser: Remeis Observatory and ECAP, Universitat Erlangen-Nurnberg
Barbara De Marco: Max-Planck-Institut fur extraterrestrische Physik
Luigi C. Gallo: Saint Mary’s University
Javier Garcia: Space Radiation Laboratory, California Institute of Technology, 1200 East California Boulevard
Fiona A. Harrison: Space Radiation Laboratory, California Institute of Technology, 1200 East California Boulevard
Ashley L. King: Kavli Institute for Particle Astrophysics and Cosmology, Stanford University
Matthew J. Middleton: School of Physics and Astronomy, University of Southampton
Jon M. Miller: University of Michigan, 1085 South University Avenue
Giovanni Miniutti: Centro de Astrobiologia (CSIC-INTA), Departimento de Astrofsica, ESAC
Christopher S. Reynolds: University of Maryland
Phil Uttley: Astronomical Institute Anton Pannekoek, University of Amsterdam
Ranjan Vasudevan: Institute of Astronomy
Dominic J. Walton: Institute of Astronomy
Daniel R. Wilkins: Kavli Institute for Particle Astrophysics and Cosmology, Stanford University
Abderahmen Zoghbi: University of Michigan, 1085 South University Avenue

Nature, 2017, vol. 543, issue 7643, 83-86

Abstract: X-ray detection of an ultrafast outflow of gas is strongly linked with energy emission from the inner accretion disk of a black hole, suggesting that X-rays ionize the outflowing disk wind.

Date: 2017
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DOI: 10.1038/nature21385

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