An increase in black hole activity in galaxies with kinematically misaligned gas
An increase in black hole activity in galaxies with kinematically misaligned gas
External accretion events such as a galaxy merger or the accretion of gas from the immediate environment of a galaxy can create a large misalignment between the gas and the stellar kinematics. Numerical simulations have suggested that misaligned structures may promote the inflow of gas to the nucleus of the galaxy and the accretion of gas by the central supermassive black hole. We show for the first time that galaxies with a strong misalignment between the ionized gas and stellar kinematic angles have a higher observed fraction of active black holes than galaxies with aligned rotation of gas and stars. The increase in black hole activity suggests that the process of formation and/or the presence of misaligned structures are connected with the fuelling of active supermassive black holes.
463–472
Raimundo, Sandra I.
e409d9d3-17e8-4049-ad29-43ada60b24e2
Malkan, Matthew
242b58b6-b6c1-467b-977a-5c5ac9376a8a
Vestergaard, Marianne
3d2377bc-0c0a-4198-9439-e7e9ac344b4e
1 April 2023
Raimundo, Sandra I.
e409d9d3-17e8-4049-ad29-43ada60b24e2
Malkan, Matthew
242b58b6-b6c1-467b-977a-5c5ac9376a8a
Vestergaard, Marianne
3d2377bc-0c0a-4198-9439-e7e9ac344b4e
Raimundo, Sandra I., Malkan, Matthew and Vestergaard, Marianne
(2023)
An increase in black hole activity in galaxies with kinematically misaligned gas.
Nature Astronomy, 7 (4), .
(doi:10.1038/s41550-022-01880-z).
Abstract
External accretion events such as a galaxy merger or the accretion of gas from the immediate environment of a galaxy can create a large misalignment between the gas and the stellar kinematics. Numerical simulations have suggested that misaligned structures may promote the inflow of gas to the nucleus of the galaxy and the accretion of gas by the central supermassive black hole. We show for the first time that galaxies with a strong misalignment between the ionized gas and stellar kinematic angles have a higher observed fraction of active black holes than galaxies with aligned rotation of gas and stars. The increase in black hole activity suggests that the process of formation and/or the presence of misaligned structures are connected with the fuelling of active supermassive black holes.
Text
An increase in black hole activity in galaxies with kinematically misaligned gas
- Accepted Manuscript
More information
Accepted/In Press date: 12 December 2022
e-pub ahead of print date: 19 January 2023
Published date: 1 April 2023
Additional Information:
arXiv:submit/4693525
Identifiers
Local EPrints ID: 476710
URI: http://eprints.soton.ac.uk/id/eprint/476710
ISSN: 2397-3366
PURE UUID: 9862e5a7-2bb8-4c79-b9de-d9412e303c98
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Date deposited: 12 May 2023 16:30
Last modified: 19 Jul 2023 04:01
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Contributors
Author:
Matthew Malkan
Author:
Marianne Vestergaard
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