The close environments of accreting massive black holes are shaped by radiative feedback

Claudio Ricci (), Benny Trakhtenbrot, Michael J. Koss, Yoshihiro Ueda, Kevin Schawinski, Kyuseok Oh, Isabella Lamperti, Richard Mushotzky, Ezequiel Treister, Luis C. Ho, Anna Weigel, Franz E. Bauer, Stephane Paltani, Andrew C. Fabian, Yanxia Xie and Neil Gehrels
Additional contact information
Claudio Ricci: Instituto de Astrofísica, Facultad de Física, Pontificia Universidad Católica de Chile
Benny Trakhtenbrot: Institute for Astronomy, ETH Zurich
Michael J. Koss: Institute for Astronomy, ETH Zurich
Yoshihiro Ueda: Kyoto University
Kevin Schawinski: Institute for Astronomy, ETH Zurich
Kyuseok Oh: Institute for Astronomy, ETH Zurich
Isabella Lamperti: Institute for Astronomy, ETH Zurich
Richard Mushotzky: University of Maryland
Ezequiel Treister: Instituto de Astrofísica, Facultad de Física, Pontificia Universidad Católica de Chile
Luis C. Ho: Kavli Institute for Astronomy and Astrophysics, Peking University
Anna Weigel: Institute for Astronomy, ETH Zurich
Franz E. Bauer: Instituto de Astrofísica, Facultad de Física, Pontificia Universidad Católica de Chile
Stephane Paltani: University of Geneva
Andrew C. Fabian: Institute of Astronomy
Yanxia Xie: Kavli Institute for Astronomy and Astrophysics, Peking University
Neil Gehrels: NASA Goddard Space Flight Center

Nature, 2017, vol. 549, issue 7673, 488-491

Abstract: Radiation pressure on dusty gas is the main physical mechanism that regulates the distribution of the circumnuclear material that obscures many supermassive black holes.

Date: 2017
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DOI: 10.1038/nature23906

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