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

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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

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