Lorentz Factors of Compact Jets in Black Hole X-Ray Binaries

Lorentz Factors of Compact Jets in Black Hole X-Ray Binaries

© 2019. The American Astronomical Society. All rights reserved.. Compact, continuously launched jets in black hole X-ray binaries (BHXBs) produce radio to optical/IR synchrotron emission. In most BHXBs, an IR excess (above the disk component) is observed when the jet is present in the hard spectral...

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Bibliographic Details
Main Authors: Saikia, P., Russell, D.M., Bramich, D.M., Miller-Jones, James, Baglio, M.C., Degenaar, N.
Format: Journal Article
Language:English
Published: IOP PUBLISHING LTD 2019
Subjects:
Science & Technology
Physical Sciences
Astronomy & Astrophysics
LENS-THIRRING PRECESSION
CANDIDATE XTE J1752-223
ACTIVE GALACTIC NUCLEI
LOW/HARD STATE
MULTIWAVELENGTH OBSERVATIONS
GX 339-4
SYNCHROTRON EMISSION
SWIFT J1753.5-0127
FUNDAMENTAL PLANE
INFRARED OBSERVATIONS
Online Access:http://purl.org/au-research/grants/arc/FT140101082
http://hdl.handle.net/20.500.11937/80167

Internet

http://purl.org/au-research/grants/arc/FT140101082
http://hdl.handle.net/20.500.11937/80167

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