An extremely powerful long-lived superluminal ejection from the black hole MAXI J1820+070

An extremely powerful long-lived superluminal ejection from the black hole MAXI J1820+070

Black holes in binary systems execute patterns of outburst activity where two characteristic X-ray states are associated with different behaviours observed at radio wavelengths. The hard state is associated with radio emission indicative of a continuously replenished, collimated, relativistic jet, w...

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Bibliographic Details
Main Authors: Bright, J.S., Fender, R.P., Motta, S.E., Williams, D.R.A., Moldon, J., Plotkin, Richard, Miller-Jones, James, Heywood, I., Tremou, E., Beswick, R., Sivakoff, G.R., Corbel, S., Buckley, D.A.H., Homan, J., Gallo, E., Tetarenko, A.J., Russell, T.D., Green, D.A., Titterington, D., Woudt, P.A., Armstrong, R.P., Groot, P.J., Horesh, A., Horst, A.J.V.D., Körding, E.G., McBride, V.A., Rowlinson, A., Wijers, R.A.M.J.
Format: Journal Article
Language:English
Published: NATURE PORTFOLIO 2020
Subjects:
Science & Technology
Physical Sciences
Astronomy & Astrophysics
X-RAY JETS
LARGE-SCALE
RELATIVISTIC JETS
XTE J1550-564
EMISSION
OUTBURST
ORIGIN
MODEL
GHZ
Online Access:http://purl.org/au-research/grants/arc/FT140101082
http://hdl.handle.net/20.500.11937/91530

Internet

http://purl.org/au-research/grants/arc/FT140101082
http://hdl.handle.net/20.500.11937/91530

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