AT2019azh: An unusually long-lived, radio-bright thermal tidal disruption event

Tidal disruption events (TDEs) occur when a star is destroyed by a supermassive black hole at the centre of a galaxy, temporarily increasing the accretion rate on to the black hole and producing a bright flare across the electromagnetic spectrum. Radio observations of TDEs trace outflows and jets th...

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Main Authors: Goodwin, A.J., Van Velzen, S., Miller-Jones, James, Mummery, A., Bietenholz, M.F., Wederfoort, A., Hammerstein, E., Bonnerot, C., Hoffmann, J., Yan, L.
Format: Journal Article
Language:English
Published: OXFORD UNIV PRESS 2022
Subjects:
Online Access:http://purl.org/au-research/grants/arc/DP200102471
http://hdl.handle.net/20.500.11937/90025
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author Goodwin, A.J.
Van Velzen, S.
Miller-Jones, James
Mummery, A.
Bietenholz, M.F.
Wederfoort, A.
Hammerstein, E.
Bonnerot, C.
Hoffmann, J.
Yan, L.
author_facet Goodwin, A.J.
Van Velzen, S.
Miller-Jones, James
Mummery, A.
Bietenholz, M.F.
Wederfoort, A.
Hammerstein, E.
Bonnerot, C.
Hoffmann, J.
Yan, L.
author_sort Goodwin, A.J.
building Curtin Institutional Repository
collection Online Access
description Tidal disruption events (TDEs) occur when a star is destroyed by a supermassive black hole at the centre of a galaxy, temporarily increasing the accretion rate on to the black hole and producing a bright flare across the electromagnetic spectrum. Radio observations of TDEs trace outflows and jets that may be produced. Radio detections of the outflows from TDEs are uncommon, with only about one-third of TDEs discovered to date having published radio detections. Here, we present over 2 yr of comprehensive, multiradio frequency monitoring observations of the TDE AT2019azh taken with the Very Large Array and MeerKAT radio telescopes from approximately 10 d pre-optical peak to 810 d post-optical peak. AT2019azh shows unusual radio emission for a thermal TDE, as it brightened very slowly over 2 yr, and showed fluctuations in the synchrotron energy index of the optically thin synchrotron emission from 450 d post-disruption. Based on the radio properties, we deduce that the outflow in this event is likely non-relativistic and could be explained by a spherical outflow arising from self-stream intersections or a mildly collimated outflow from accretion on to the supermassive black hole. This data set provides a significant contribution to the observational data base of outflows from TDEs, including the earliest radio detection of a non-relativistic TDE to date, relative to the optical discovery.
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spelling curtin-20.500.11937-900252023-02-07T07:19:02Z AT2019azh: An unusually long-lived, radio-bright thermal tidal disruption event Goodwin, A.J. Van Velzen, S. Miller-Jones, James Mummery, A. Bietenholz, M.F. Wederfoort, A. Hammerstein, E. Bonnerot, C. Hoffmann, J. Yan, L. Science & Technology Physical Sciences Astronomy & Astrophysics radio continuum: transients transients: tidal disruption events X-RAY BLACK-HOLE DISC FORMATION STAR JET CANDIDATE EMISSION FLARES MULTIWAVELENGTH OUTBURST Tidal disruption events (TDEs) occur when a star is destroyed by a supermassive black hole at the centre of a galaxy, temporarily increasing the accretion rate on to the black hole and producing a bright flare across the electromagnetic spectrum. Radio observations of TDEs trace outflows and jets that may be produced. Radio detections of the outflows from TDEs are uncommon, with only about one-third of TDEs discovered to date having published radio detections. Here, we present over 2 yr of comprehensive, multiradio frequency monitoring observations of the TDE AT2019azh taken with the Very Large Array and MeerKAT radio telescopes from approximately 10 d pre-optical peak to 810 d post-optical peak. AT2019azh shows unusual radio emission for a thermal TDE, as it brightened very slowly over 2 yr, and showed fluctuations in the synchrotron energy index of the optically thin synchrotron emission from 450 d post-disruption. Based on the radio properties, we deduce that the outflow in this event is likely non-relativistic and could be explained by a spherical outflow arising from self-stream intersections or a mildly collimated outflow from accretion on to the supermassive black hole. This data set provides a significant contribution to the observational data base of outflows from TDEs, including the earliest radio detection of a non-relativistic TDE to date, relative to the optical discovery. 2022 Journal Article http://hdl.handle.net/20.500.11937/90025 10.1093/mnras/stac333 English http://purl.org/au-research/grants/arc/DP200102471 http://creativecommons.org/licenses/by/4.0/ OXFORD UNIV PRESS fulltext
spellingShingle Science & Technology
Physical Sciences
Astronomy & Astrophysics
radio continuum: transients
transients: tidal disruption events
X-RAY
BLACK-HOLE
DISC FORMATION
STAR
JET
CANDIDATE
EMISSION
FLARES
MULTIWAVELENGTH
OUTBURST
Goodwin, A.J.
Van Velzen, S.
Miller-Jones, James
Mummery, A.
Bietenholz, M.F.
Wederfoort, A.
Hammerstein, E.
Bonnerot, C.
Hoffmann, J.
Yan, L.
AT2019azh: An unusually long-lived, radio-bright thermal tidal disruption event
title AT2019azh: An unusually long-lived, radio-bright thermal tidal disruption event
title_full AT2019azh: An unusually long-lived, radio-bright thermal tidal disruption event
title_fullStr AT2019azh: An unusually long-lived, radio-bright thermal tidal disruption event
title_full_unstemmed AT2019azh: An unusually long-lived, radio-bright thermal tidal disruption event
title_short AT2019azh: An unusually long-lived, radio-bright thermal tidal disruption event
title_sort at2019azh: an unusually long-lived, radio-bright thermal tidal disruption event
topic Science & Technology
Physical Sciences
Astronomy & Astrophysics
radio continuum: transients
transients: tidal disruption events
X-RAY
BLACK-HOLE
DISC FORMATION
STAR
JET
CANDIDATE
EMISSION
FLARES
MULTIWAVELENGTH
OUTBURST
url http://purl.org/au-research/grants/arc/DP200102471
http://hdl.handle.net/20.500.11937/90025