SIMBAD references

2016MNRAS.463..628R - Mon. Not. R. Astron. Soc., 463, 628-634 (2016/November-3)

Disc-jet quenching of the galactic black hole Swift J1753.5-0127.

RUSHTON A.P., SHAW A.W., FENDER R.P., ALTAMIRANO D., GANDHI P., UTTLEY P., CHARLES P.A., KOLEHMAINEN M., ANDERSON G.E., RUMSEY C. and TITTERINGTON D.J.

Abstract (from CDS):

We report on radio and X-ray monitoring observations of the BHC Swift J1753.5-0127 taken over a ∼10 yr period. Presented are daily radio observations at 15 GHz with the Arcminute Microkelvin Imager Large Array (AMI-LA) and X-ray data from Swift X-ray Telescope and Burst Alert Telescope. Also presented is a deep 2 h JVLA observation taken in an unusually low-luminosity soft-state (with a low disc temperature). We show that although the source has remained relatively radio-quiet compared to XRBs with a similar X-ray luminosity in the hard-state, the power-law relationship scales as ζ = 0.96 ± 0.06, i.e. slightly closer to what has been considered for radiatively inefficient accretion discs. We also place the most stringent limit to date on the radio-jet quenching in an XRB soft-state, showing the connection of the jet quenching to the X-ray power-law component; the radio flux in the soft-state was found to be < 21 µJy, which is a quenching factor of >= 25.

Abstract Copyright: © 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): accretion, accretion discs - time - stars: black holes - stars: jets - radio continuum: stars - X-rays: binaries

Simbad objects: 27

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2021.03.01-17:29:11

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