Flavors of Relativistic Jets from Black Hole Binaries

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Bibliographic Details
Main Author:	Sthepane Corbel
Format:	Artículo científico
Language:	en
Published:	Universidad Nacional Autónoma de México 2007
Subjects:	Física, Astronomía y Matemáticas Black hole physics ISM: jets and outflows radio continuum: stars
Online Access:	Acceder al recurso
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author	Sthepane Corbel
author_facet	Sthepane Corbel
contents	Flavors of Relativistic Jets from Black Hole Binaries Sthepane Corbel Física, Astronomía y Matemáticas Black hole physics ISM: jets and outflows radio continuum: stars Relativistic jets are now believed to be a fairly ubiquitous property of accreting compact objects, and areintimately coupled with the accretion history. Associated with rapid changes in the accretion states of thebinary systems, ejections of relativistic plasma can be observed at radio frequencies on timescale of weeksbefore becoming undetectable. Recent observations point to long term effects of these ejecta on the interstellar medium with the formation of large scale lobes around binary systems and the acceleration of particles up to very high energy. 2007 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57102713 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.27
format	Artículo científico
id	redalyc_57102713
language	en
publishDate	2007
publisher	Universidad Nacional Autónoma de México
spellingShingle	Flavors of Relativistic Jets from Black Hole Binaries Sthepane Corbel Física, Astronomía y Matemáticas Black hole physics ISM: jets and outflows radio continuum: stars Flavors of Relativistic Jets from Black Hole Binaries Sthepane Corbel Física, Astronomía y Matemáticas Black hole physics ISM: jets and outflows radio continuum: stars Relativistic jets are now believed to be a fairly ubiquitous property of accreting compact objects, and areintimately coupled with the accretion history. Associated with rapid changes in the accretion states of thebinary systems, ejections of relativistic plasma can be observed at radio frequencies on timescale of weeksbefore becoming undetectable. Recent observations point to long term effects of these ejecta on the interstellar medium with the formation of large scale lobes around binary systems and the acceleration of particles up to very high energy. 2007 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57102713 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.27
title	Flavors of Relativistic Jets from Black Hole Binaries
topic	Física, Astronomía y Matemáticas Black hole physics ISM: jets and outflows radio continuum: stars
url	https://www.redalyc.org/articulo.oa?id=57102713

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