A rapidly changing jet orientation in the stellar-mass black-hole system V404 Cygni

A rapidly changing jet orientation in the stellar-mass black-hole system V404 Cygni

© 2019, The Author(s), under exclusive licence to Springer Nature Limited. Powerful relativistic jets are one of the main ways in which accreting black holes provide kinetic feedback to their surroundings. Jets launched from or redirected by the accretion flow that powers them are expected to be aff...

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Bibliographic Details
Main Authors: Miller-Jones, James, Tetarenko, A.J., Sivakoff, G.R., Middleton, M.J., Altamirano, D., Anderson, Gemma, Belloni, T.M., Fender, R.P., Jonker, P.G., Körding, E.G., Krimm, H.A., Maitra, D., Markoff, S., Migliari, S., Mooley, K.P., Rupen, M.P., Russell, D.M., Russell, T.D., Sarazin, C.L., Soria, R., Tudose, V.
Format: Journal Article
Language:English
Published: NATURE PUBLISHING GROUP 2019
Subjects:
Science & Technology
Multidisciplinary Sciences
Science & Technology - Other Topics
LENS-THIRRING PRECESSION
WARPED ACCRETION DISCS
X-RAY
EVOLUTION
OUTBURST
MODELS
BASE
ULXS
Online Access:http://purl.org/au-research/grants/arc/FT140101082
http://hdl.handle.net/20.500.11937/80100

Internet

http://purl.org/au-research/grants/arc/FT140101082
http://hdl.handle.net/20.500.11937/80100

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