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The role of outflows in black-hole X-ray binaries

Published online by Cambridge University Press:  28 October 2024

Nikolaos D. Kylafis Open the ORCID record for Nikolaos D. Kylafis [Opens in a new window]  and
Pablo Reig
Nikolaos D. Kylafis*
Affiliation:
University of Crete, Physics Department, 70013 Heraklion, Greece Institute of Astrophysics, FORTH, 70013 Heraklion, Greece
Pablo Reig*
Affiliation:
University of Crete, Physics Department, 70013 Heraklion, Greece Institute of Astrophysics, FORTH, 70013 Heraklion, Greece
*
email: kylafis@physics.uoc.gr
email: pau@physics.uoc.gr
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Abstract

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. An outflow, from the hot inner flow, in black-hole X-ray binaries is always expected due to the positive Bernoulli integral in the hot inner flow. We have demonstrated that, if one considers this outflow as the place where not only Comptonization occurs, but also radio emission, many observed correlations, including the long-standing one between radio and X-rays, can be explained with one simple model.

Keywords

X-ray binariesblack holesoutflowsjets
Type
Contributed Paper
Information
Proceedings of the International Astronomical Union , Volume 19 , Symposium S378: Black Hole Winds at All Scales , December 2023 , pp. 87 - 89
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Creative Commons
Creative Common License - CCCreative Common License - BY
This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted re-use, distribution and reproduction, provided the original article is properly cited.
Copyright
© The Author(s), 2024. Published by Cambridge University Press on behalf of International Astronomical Union

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