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Super Winds and Radio Emission in X-ray Binary Systems
High Energy Astrophysical Phenomena · Submitted 25 Nov 2023
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim We have recently proposed that supercritical colliding wind binaries (SCWBs) are suitable scenarios for particle acceleration and nonthermal radiation.
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The abstract, sentence by sentence
We have recently proposed that supercritical colliding wind binaries (SCWBs) are suitable scenarios for particle acceleration and nonthermal radiation. In these X-ray binary systems (XRBs), the wind from the companion star collides with the wind ejected from the super-Eddington accretion disk of the stellar black hole. Strong shocks are generated in this collision, leading to the acceleration of particles and subsequent broadband emission through different nonthermal radiative processes. In particular, we estimate luminosities of the order of $L\approx 10^{34}\,{\rm erg\,s^{-1}}$ in the radio band. One of the major components in these processes is the power provided by the super wind expelled from the disk. Furthermore, some properties of the wind photosphere, such as its geometry or its temperature distribution, also contribute to the absorption and reprocessing of the nonthermal radiation. In this work, we perform a more detailed description of the powerful wind launched from the accretion disk, in order to obtain a better understanding of the above-mentioned processes.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | We have recently proposed that supercritical colliding wind binaries (SCWBs) are suitable scenarios for particle acceleration and nonthermal radiation. | background 0.78 | 0.74 | 0.40 | hedged possibility 0.80 |
| s1 | In these X-ray binary systems (XRBs), the wind from the companion star collides with the wind ejected from the super-Eddington accretion disk of the stellar black hole. | background 0.99 | 0.10 | 0.05 | asserted 1.00 |
| s2 | Strong shocks are generated in this collision, leading to the acceleration of particles and subsequent broadband emission through different nonthermal radiative processes. | background 0.87 | 0.19 | 0.13 | asserted 1.00 |
| s3 | In particular, we estimate luminosities of the order of $L\approx 10^{34}\,{\rm erg\,s^{-1}}$ in the radio band. | result 0.96 | 0.88 | 0.21 | asserted 0.52 |
| s4 | One of the major components in these processes is the power provided by the super wind expelled from the disk. | background 0.85 | 0.18 | 0.08 | asserted 0.99 |
| s5 | Furthermore, some properties of the wind photosphere, such as its geometry or its temperature distribution, also contribute to the absorption and reprocessing of the nonthermal radiation. | background 0.92 | 0.12 | 0.04 | asserted 0.68 |
| s6 | In this work, we perform a more detailed description of the powerful wind launched from the accretion disk, in order to obtain a better understanding of the above-mentioned processes. | contribution 1.00 | 0.90 | 0.09 | asserted 0.94 |
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Original abstract
We have recently proposed that supercritical colliding wind binaries (SCWBs) are suitable scenarios for particle acceleration and nonthermal radiation. In these X-ray binary systems (XRBs), the wind from the companion star collides with the wind ejected from the super-Eddington accretion disk of the stellar black hole. Strong shocks are generated in this collision, leading to the acceleration of particles and subsequent broadband emission through different nonthermal radiative processes. In particular, we estimate luminosities of the order of $L\approx 10^{34}\,{\rm erg\,s^{-1}}$ in the radio band. One of the major components in these processes is the power provided by the super wind expelled from the disk. Furthermore, some properties of the wind photosphere, such as its geometry or its temperature distribution, also contribute to the absorption and reprocessing of the nonthermal radiation. In this work, we perform a more detailed description of the powerful wind launched from the accretion disk, in order to obtain a better understanding of the above-mentioned processes.
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4 arXiv papers cite this in 5 sentences
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The height of the apparent photosphere from the equatorial plane, $z_ph$, can be calculated by solving the integral [ref] [equation]
Effects of Bethe-Heitler pair production in ultraluminous X-ray sources · Wind of the disk · 0.91
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