Rapid Accretion State Transitions following the Tidal Disruption Event AT2018fyk

Rapid Accretion State Transitions following the Tidal Disruption Event AT2018fyk

Following a tidal disruption event (TDE), the accretion rate can evolve from quiescent to near-Eddington levels and back over timescales of months to years. This provides a unique opportunity to study the formation and evolution of the accretion flow around supermassive black holes (SMBHs). We prese...

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Bibliographic Details
Main Authors: Wevers, T., Pasham, D.R., Van Velzen, S., Miller-Jones, James, Uttley, P., Gendreau, K.C., Remillard, R., Arzoumanian, Z., Löwenstein, M., Chiti, A.
Format: Journal Article
Language:English
Published: IOP Publishing Ltd 2021
Subjects:
Science & Technology
Physical Sciences
Astronomy & Astrophysics
ACTIVE GALACTIC NUCLEI
X-RAY BINARIES
BLACK-HOLE MASSES
FUNDAMENTAL PLANE
POWER SPECTRA
COMPACT JET
STELLAR
EVOLUTION
VARIABILITY
AGN
Online Access:http://purl.org/au-research/grants/arc/DP200102471
http://hdl.handle.net/20.500.11937/90030

Internet

http://purl.org/au-research/grants/arc/DP200102471
http://hdl.handle.net/20.500.11937/90030

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