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High-energy emission from accreting black holes with high-mass donor stars

Document type: Articulo

Abstract

We present an analysis of the interactions of a distribution of relativistic protons under the typical conditions of the corona surrounding an accreting black hole. The model is applied to a concrete binary system with a high-mass donor star: the classical source Cygnus X-1

General information

Issue date: diciembre 2008
Document language: English
Journal: Revista Mexicana de Astronomía y Astrofísica; vol. 33
Origin: Facultad de Ciencias Astronómicas y Geofísicas
Others identifiers: hdl:11336/22920
ISSN: 0185-1101
Pages: 122-122
xmlui.dri2xhtml.METS-1.0.item-dc-subject: Cygnus x-1 ; Relativistic protons ; Binary systems
Subjects: Ciencias Astronómicas

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Created: 4 de junio de 2020
Available since: 4 de junio de 2020
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  • http://sedici.unlp.edu.ar/handle/10915/97510

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    Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Except where otherwise noted, this item's license is described as Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)