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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Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_03796566_v_n552_p175_Mirabel |
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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 |
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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 |
_version_ |
1807320067935830016 |