Coupling between the accreting corona and the relativistic jet in the micro quasar GRS 1915+105
Mariano Mendez (Univ. of Groningen), Konstantinos Karpouzas (Univ. of, Groningen, Univ. of Southampton), Federico Garcia (Univ. of Groningen, IAR),, Liang Zhang (Univ. of Southampton), Yuexin Zhang (Univ. of Groningen), Tomaso, M. Belloni (INAF)

TL;DR
This study reveals a strong, long-term coupling between the accretion disc, corona, and jet in GRS 1915+105, showing energy transfer between the X-ray corona and the relativistic jet over a decade.
Contribution
It provides the first direct evidence that the energy powering the corona and jet in GRS 1915+105 is interchangeable, demonstrating the corona morphs into the jet.
Findings
Radio flux correlates with iron line flux and corona temperature.
Anti-correlation between radio flux and corona temperature.
Correlations persist over approximately 10 years.
Abstract
GRS 1915+105 was the first stellar-mass black-hole in our Galaxy to display a superluminal radio jet, similar to those observed in active galactic nuclei with a supermassive black hole at the centre. It has been proposed that the radio emission in GRS 1915+105 is fed by instabilities in the accretion disc by which the inner parts of the accretion flow is ejected in the jet. Here we show that there is a significant correlation between: (i) the radio flux, coming from the jet, and the flux of the iron emission line, coming from the disc and, (ii) the temperature of the corona that produces the high-energy part of the X-ray spectrum via inverse Compton scattering and the amplitude of a high-frequency variability component coming from the innermost part of the accretion flow. At the same time, the radio flux and the flux of the iron line are strongly anti-correlated with the temperature of…
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