Radio Variability from a Quiescent Stellar-mass Black Hole Jet

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Radio Variability from a Quiescent Stellar-mass Black Hole Jet

© 2019 The American Astronomical Society. All rights reserved. Relativistic outflows are believed to be a common feature of black hole X-ray binaries (BHXBs) at the lowest accretion rates, when they are in their "quiescent" spectral state. However, we still lack a detailed understanding o...

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Bibliographic Details
Main Authors:	Plotkin, Richard, Miller-Jones, James, Chomiuk, L., Strader, J., Bruzewski, S., Bundas, A., Smith, K.R., Ruan, J.J.
Format:	Journal Article
Language:	English
Published:	IOP PUBLISHING LTD 2019
Subjects:	Science & Technology Physical Sciences Astronomy & Astrophysics accretion, accretion disks stars: black holes stars: individual (V404 Cygni) X-rays: binaries X-RAY BINARIES ACTIVE GALACTIC NUCLEI NOVA V404 CYGNI NEUTRON-STAR LIGHT CURVES RELATIVISTIC JETS FLUX CORRELATION ACCRETION FLOWS COMPLETE SAMPLE XTE J1550-564
Online Access:	http://purl.org/au-research/grants/arc/FT140101082 http://hdl.handle.net/20.500.11937/80173

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