Microquasar-agn-grb connections

I review the progress made on the physics of black hole systems in the context of the analogy between AGN and microquasars that was proposed one decade ago. If the emerging empirical correlations between the observational properties of stellar and supermassive black holes will become more robust, we...

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Detalles Bibliográficos
Autores principales: Mirabel, I.E., Schonfelder V., Lichti G., Winkler C.
Formato: CONF
Materias:
AGN
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_03796566_v_n552_p175_Mirabel
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spelling todo:paper_03796566_v_n552_p175_Mirabel2023-10-03T15:33:32Z Microquasar-agn-grb connections Mirabel, I.E. Schonfelder V. Lichti G. Winkler C. Binaries: AGN Black holes: x-rays Correlation methods Cosmic rays Gamma rays Hydrodynamics Mathematical models Surveys AGN Binaries Black holes Galactic Plane Survey (GPS) X-rays Astronomy I review the progress made on the physics of black hole systems in the context of the analogy between AGN and microquasars that was proposed one decade ago. If the emerging empirical correlations between the observational properties of stellar and supermassive black holes will become more robust, we will use them to determine the mass and spin of black holes, independently of theoretical models. Microquasars are fossils of sources of Gamma-ray bursts (GRBs) of long duration, and their kinematics provides observational clues on the physics of collapsars. If jets in GRBs, microquasars and AGN are due to a unique universal magnetohydrodynamic mechanism, synergy between the research on these three different classes of cosmic objects will lead to further progress in black hole physics and astrophysics. The potential contributions with INTEGRAL in this field of research are also discussed. It is shown that the Galactic Plane Survey (GPS) with INTEGRAL is unraveling new extragalactic sources of hard x-rays behind the Milky Way, as well as new black hole high-mass binaries that were hidden by large columns of gas and dust. CONF info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_03796566_v_n552_p175_Mirabel
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic Binaries: AGN
Black holes: x-rays
Correlation methods
Cosmic rays
Gamma rays
Hydrodynamics
Mathematical models
Surveys
AGN
Binaries
Black holes
Galactic Plane Survey (GPS)
X-rays
Astronomy
spellingShingle Binaries: AGN
Black holes: x-rays
Correlation methods
Cosmic rays
Gamma rays
Hydrodynamics
Mathematical models
Surveys
AGN
Binaries
Black holes
Galactic Plane Survey (GPS)
X-rays
Astronomy
Mirabel, I.E.
Schonfelder V.
Lichti G.
Winkler C.
Microquasar-agn-grb connections
topic_facet Binaries: AGN
Black holes: x-rays
Correlation methods
Cosmic rays
Gamma rays
Hydrodynamics
Mathematical models
Surveys
AGN
Binaries
Black holes
Galactic Plane Survey (GPS)
X-rays
Astronomy
description I review the progress made on the physics of black hole systems in the context of the analogy between AGN and microquasars that was proposed one decade ago. If the emerging empirical correlations between the observational properties of stellar and supermassive black holes will become more robust, we will use them to determine the mass and spin of black holes, independently of theoretical models. Microquasars are fossils of sources of Gamma-ray bursts (GRBs) of long duration, and their kinematics provides observational clues on the physics of collapsars. If jets in GRBs, microquasars and AGN are due to a unique universal magnetohydrodynamic mechanism, synergy between the research on these three different classes of cosmic objects will lead to further progress in black hole physics and astrophysics. The potential contributions with INTEGRAL in this field of research are also discussed. It is shown that the Galactic Plane Survey (GPS) with INTEGRAL is unraveling new extragalactic sources of hard x-rays behind the Milky Way, as well as new black hole high-mass binaries that were hidden by large columns of gas and dust.
format CONF
author Mirabel, I.E.
Schonfelder V.
Lichti G.
Winkler C.
author_facet Mirabel, I.E.
Schonfelder V.
Lichti G.
Winkler C.
author_sort Mirabel, I.E.
title Microquasar-agn-grb connections
title_short Microquasar-agn-grb connections
title_full Microquasar-agn-grb connections
title_fullStr Microquasar-agn-grb connections
title_full_unstemmed Microquasar-agn-grb connections
title_sort microquasar-agn-grb connections
url http://hdl.handle.net/20.500.12110/paper_03796566_v_n552_p175_Mirabel
work_keys_str_mv AT mirabelie microquasaragngrbconnections
AT schonfelderv microquasaragngrbconnections
AT lichtig microquasaragngrbconnections
AT winklerc microquasaragngrbconnections
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