Non-thermal processes around accreting galactic black holes
Context. Accreting black holes in galactic X-ray sources are surrounded by hot plasma. The innermost part of these systems is likely a corona with different temperatures for ions and electrons. In the so-called low-hard state, hot electrons Comptonize soft X-ray photons from the disk that partially...
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| Formato: | Articulo |
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2010
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| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/82513 |
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I19-R120-10915-82513 |
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dspace |
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Universidad Nacional de La Plata |
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I-19 |
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R-120 |
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SEDICI (UNLP) |
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Inglés |
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Ciencias Astronómicas Gamma rays: general Radiation mechanisms: non-thermal X-rays: binaries |
| spellingShingle |
Ciencias Astronómicas Gamma rays: general Radiation mechanisms: non-thermal X-rays: binaries Romero, Gustavo Esteban Vieyro, Florencia Laura Vila, Gabriela Soledad Non-thermal processes around accreting galactic black holes |
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Ciencias Astronómicas Gamma rays: general Radiation mechanisms: non-thermal X-rays: binaries |
| description |
Context. Accreting black holes in galactic X-ray sources are surrounded by hot plasma. The innermost part of these systems is likely a corona with different temperatures for ions and electrons. In the so-called low-hard state, hot electrons Comptonize soft X-ray photons from the disk that partially penetrates the corona, producing emission up to ∼150 keV, well beyond the expectations for an optically thick disk of maximum temperature ∼10<SUP>7</SUP> K. However, sources such as Cygnus X-1 produce steady emission up to a few MeV, which is indicative of a non-thermal contribution to the spectral energy distribution.
Aims. We study the radiative output produced by the injection of non-thermal (both electron and proton) particles in a magnetized corona around a black hole.
Methods. Energy losses and maximum energies are estimated for all types of particles in a variety of models, characterized by different kinds of advection and relativistic proton content. Transport equations are solved for primary and secondary particles, and spectral energy distributions are determined and corrected by internal absorption.
Results. We show that a local injection of non-thermal particles can account for the high energy excess observed in some sources, and we predict the existence of a high-energy bump at energies above 1 TeV, and typical luminosities of ∼10<SUP>33</SUP> erg s<SUP>-1</SUP>.
Conclusions. High-energy instruments such as the future Cherenkov Telescope Array (CTA) can be used to probe the relativistic particle content of the coronae around galactic black holes. |
| format |
Articulo Articulo |
| author |
Romero, Gustavo Esteban Vieyro, Florencia Laura Vila, Gabriela Soledad |
| author_facet |
Romero, Gustavo Esteban Vieyro, Florencia Laura Vila, Gabriela Soledad |
| author_sort |
Romero, Gustavo Esteban |
| title |
Non-thermal processes around accreting galactic black holes |
| title_short |
Non-thermal processes around accreting galactic black holes |
| title_full |
Non-thermal processes around accreting galactic black holes |
| title_fullStr |
Non-thermal processes around accreting galactic black holes |
| title_full_unstemmed |
Non-thermal processes around accreting galactic black holes |
| title_sort |
non-thermal processes around accreting galactic black holes |
| publishDate |
2010 |
| url |
http://sedici.unlp.edu.ar/handle/10915/82513 |
| work_keys_str_mv |
AT romerogustavoesteban nonthermalprocessesaroundaccretinggalacticblackholes AT vieyroflorencialaura nonthermalprocessesaroundaccretinggalacticblackholes AT vilagabrielasoledad nonthermalprocessesaroundaccretinggalacticblackholes |
| bdutipo_str |
Repositorios |
| _version_ |
1764820488357412867 |