Jet-dominated quiescent state in black hole X-ray binaries: the cases of A0620−00 and XTE J1118+480
Author:
Publisher
IOP Publishing
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/1674-4527/16/i=4/a=010/pdf
Reference80 articles.
1. States and Transitions in Black Hole Binaries
2. Characterizing the quiescent X-ray variability of the black hole low-mass X-ray binary V404 Cyg
3. Influence of Ohmic Heating on Advection-dominated Accretion Flows
4. On particle energization in accretion flows
5. THE INCLINATION OF THE SOFT X-RAY TRANSIENT A0620–00 AND THE MASS OF ITS BLACK HOLE
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1. An Observational Signature of Sub-equipartition Magnetic Fields in the Spectra of Black Hole Binaries;The Astrophysical Journal;2021-07-28
2. Swift/XRT, Chandra, and XMM–Newton observations of IGR J17091–3624 as it returns into quiescence;Monthly Notices of the Royal Astronomical Society;2020-07-10
3. Effect of magnetic flux advection on the dynamics of shock in accretion flow around a rotating black hole;Research in Astronomy and Astrophysics;2020-03-01
4. Polarized synchrotron emission in quiescent black hole X-ray transients;Monthly Notices of the Royal Astronomical Society;2016-08-26
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