Towards a larger sample of radio jets from quiescent black hole X-ray binaries

Towards a larger sample of radio jets from quiescent black hole X-ray binaries

Quiescent black hole X-ray binaries (X-ray luminosities ≲1034 erg s−1) are believed to be fed by hot accretion flows that launch compact, relativistic jets. However, due to their low luminosities, quiescent jets have been detected in the radio waveband from only five systems so far. Here, we present...

Full description

Bibliographic Details
Main Authors: Plotkin, Richard, Bahramian, Arash, Miller-Jones, James, Reynolds, M.T., Atri, P., Maccarone, T.J., Shaw, A.W., Gandhi, P.
Format: Journal Article
Language:English
Published: OXFORD UNIV PRESS 2021
Subjects:
Science & Technology
Physical Sciences
Astronomy & Astrophysics
stars: individual: BW Cir
stars: individual: GS 1124-684
X-rays: binaries
V404 CYGNI
GS 1354-64
MILKY-WAY
ACCRETION
EMISSION
STATE
VARIABILITY
ADVECTION-DOMINATED ACCRETION
HARD-STATE
FLUX CORRELATION
GX 339-4
OUTBURST
DISTANCES
A0620-00
astro-ph.HE
Online Access:http://purl.org/au-research/grants/arc/FT140101082
http://hdl.handle.net/20.500.11937/91522

Internet

http://purl.org/au-research/grants/arc/FT140101082
http://hdl.handle.net/20.500.11937/91522

Similar Items