A radio jet from the optical and X-ray bright stellar tidal disruption flare ASASSN-14li.

The tidal disruption of a star by a supermassive black hole leads to a short-lived thermal flare. Despite extensive searches, radio follow-up observations of known thermal stellar tidal disruption flares (TDFs) have not yet produced a conclusive detection. We present a detection of variable radio em...

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Main Authors: van Velzen, S., Anderson, Gemma, Stone, N., Fraser, M., Wevers, T., Metzger, B., Jonker, P., van der Horst, A., Staley, T., Mendez, A., Miller-Jones, J., Hodgkin, S., Campbell, H., Fender, R.
Format: Journal Article
Published: 2015
Online Access:http://purl.org/au-research/grants/arc/FT140101082
http://hdl.handle.net/20.500.11937/20129
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author van Velzen, S.
Anderson, Gemma
Stone, N.
Fraser, M.
Wevers, T.
Metzger, B.
Jonker, P.
van der Horst, A.
Staley, T.
Mendez, A.
Miller-Jones, J.
Hodgkin, S.
Campbell, H.
Fender, R.
author_facet van Velzen, S.
Anderson, Gemma
Stone, N.
Fraser, M.
Wevers, T.
Metzger, B.
Jonker, P.
van der Horst, A.
Staley, T.
Mendez, A.
Miller-Jones, J.
Hodgkin, S.
Campbell, H.
Fender, R.
author_sort van Velzen, S.
building Curtin Institutional Repository
collection Online Access
description The tidal disruption of a star by a supermassive black hole leads to a short-lived thermal flare. Despite extensive searches, radio follow-up observations of known thermal stellar tidal disruption flares (TDFs) have not yet produced a conclusive detection. We present a detection of variable radio emission from a thermal TDF, which we interpret as originating from a newly-launched jet. The multi-wavelength properties of the source present a natural analogy with accretion state changes of stellar mass black holes, suggesting all TDFs could be accompanied by a jet. In the rest frame of the TDF, our radio observations are an order of magnitude more sensitive than nearly all previous upper limits, explaining how these jets, if common, could thus far have escaped detection.
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institution Curtin University Malaysia
institution_category Local University
last_indexed 2025-11-14T07:33:24Z
publishDate 2015
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spelling curtin-20.500.11937-201292020-07-29T09:43:25Z A radio jet from the optical and X-ray bright stellar tidal disruption flare ASASSN-14li. van Velzen, S. Anderson, Gemma Stone, N. Fraser, M. Wevers, T. Metzger, B. Jonker, P. van der Horst, A. Staley, T. Mendez, A. Miller-Jones, J. Hodgkin, S. Campbell, H. Fender, R. The tidal disruption of a star by a supermassive black hole leads to a short-lived thermal flare. Despite extensive searches, radio follow-up observations of known thermal stellar tidal disruption flares (TDFs) have not yet produced a conclusive detection. We present a detection of variable radio emission from a thermal TDF, which we interpret as originating from a newly-launched jet. The multi-wavelength properties of the source present a natural analogy with accretion state changes of stellar mass black holes, suggesting all TDFs could be accompanied by a jet. In the rest frame of the TDF, our radio observations are an order of magnitude more sensitive than nearly all previous upper limits, explaining how these jets, if common, could thus far have escaped detection. 2015 Journal Article http://hdl.handle.net/20.500.11937/20129 10.1126/science.aad1182 http://purl.org/au-research/grants/arc/FT140101082 fulltext
spellingShingle van Velzen, S.
Anderson, Gemma
Stone, N.
Fraser, M.
Wevers, T.
Metzger, B.
Jonker, P.
van der Horst, A.
Staley, T.
Mendez, A.
Miller-Jones, J.
Hodgkin, S.
Campbell, H.
Fender, R.
A radio jet from the optical and X-ray bright stellar tidal disruption flare ASASSN-14li.
title A radio jet from the optical and X-ray bright stellar tidal disruption flare ASASSN-14li.
title_full A radio jet from the optical and X-ray bright stellar tidal disruption flare ASASSN-14li.
title_fullStr A radio jet from the optical and X-ray bright stellar tidal disruption flare ASASSN-14li.
title_full_unstemmed A radio jet from the optical and X-ray bright stellar tidal disruption flare ASASSN-14li.
title_short A radio jet from the optical and X-ray bright stellar tidal disruption flare ASASSN-14li.
title_sort radio jet from the optical and x-ray bright stellar tidal disruption flare asassn-14li.
url http://purl.org/au-research/grants/arc/FT140101082
http://hdl.handle.net/20.500.11937/20129