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Revista científica

Radiation from hot accretion flows onto black holes

Gutiérrez, Eduardo Mario et al · Asociación Argentina de Astronomía · 2020

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The hot accretion flows upon black holes are usually optically thin two-temperature plasmas inwhich electrons can achieve temperatures up to 1010 K, producing radiation via synchrotron, bremsstrahlung andinverse Compton, and the ions can reach temperatures up to 1012 K. The hottest ions might produce gammaemission through proton-proton interactions. In this work, we considered a particular model of a hot accretionflow and estimate the spectral energy distributions produced by both species of particles. Fil: Gutiérrez, Eduardo Mario. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina Fil: Vieyro, Florencia Laura. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina

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APA 7

Gutiérrez, E. M. E. A. (2020). Radiation from hot accretion flows onto black holes. http://hdl.handle.net/11336/172212

MLA

Gutiérrez, Eduardo Mario et al. "Radiation from hot accretion flows onto black holes." 2020. http://hdl.handle.net/11336/172212.

Chicago

Gutiérrez, Eduardo Mario et al. 2020. "Radiation from hot accretion flows onto black holes.". http://hdl.handle.net/11336/172212.

Harvard

Gutiérrez, E. M. E. A. 2020, Radiation from hot accretion flows onto black holes, Asociación Argentina de Astronomía, available at: http://hdl.handle.net/11336/172212 [Accessed 8 Aug. 2026].

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Title
Radiation from hot accretion flows onto black holes
Author / contributors
Gutiérrez, Eduardo Mario et al
Publisher
Asociación Argentina de Astronomía
Publication year
2020
ISSN
0571-3285
ISSN
0571-3285
Language
English

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