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

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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...

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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

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