Radio Variability from a Quiescent Stellar-mass Black Hole Jet

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...

Full description

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

Internet

http://purl.org/au-research/grants/arc/FT140101082
http://hdl.handle.net/20.500.11937/80173

Similar Items