Stellar black holes: Cosmic history and feedback at the dawn of the universe

Significant historic cosmic evolution for the formation rate of stellar black holes is inferred from current theoretical models of the evolution of massive stars, the multiple observations of compact stellar remnants in the near and distant universe, and the cosmic chemical evolution. The mean mass...

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Detalles Bibliográficos
Autores principales:	Mirabel, I.F., Romero G.E., Sunyaev R.A., Belloni T.M.
Formato:	SER
Materias:	Black holes Cosmology Microquasars
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_17439213_v6_nS275_p3_Mirabel
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

id	todo:paper_17439213_v6_nS275_p3_Mirabel
record_format	dspace
spelling	todo:paper_17439213_v6_nS275_p3_Mirabel2023-10-03T16:31:37Z Stellar black holes: Cosmic history and feedback at the dawn of the universe Mirabel, I.F. Romero G.E. Sunyaev R.A. Sunyaev R.A. Belloni T.M. Black holes Cosmology Microquasars Significant historic cosmic evolution for the formation rate of stellar black holes is inferred from current theoretical models of the evolution of massive stars, the multiple observations of compact stellar remnants in the near and distant universe, and the cosmic chemical evolution. The mean mass of stellar black holes, the fraction of black holes/neutron stars, and the fraction of black hole high mass X-ray binaries (BH-HMXBs)/solitary black holes increase with redshift. The energetic feedback from large populations of BH-HMXBs form in the first generations of star burst galaxies has been overlooked in most cosmological models of the reionization epoch of the universe. The powerful radiation, jets, and winds from BH-HMXBs heat the intergalactic medium over large volumes of space and keep it ionized until AGN take over. It is concluded that stellar black holes constrained the properties of the faintest galaxies at high redshifts. I present here the theoretical and observational grounds for the historic cosmic evolution of stellar black holes. Detailed calculations on their cosmic impact are presented elsewhere (Mirabel, Dijkstra, Laurent, Loeb, & Pritchard 2011). © International Astronomical Union 2011. SER info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_17439213_v6_nS275_p3_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	Black holes Cosmology Microquasars
spellingShingle	Black holes Cosmology Microquasars Mirabel, I.F. Romero G.E. Sunyaev R.A. Sunyaev R.A. Belloni T.M. Stellar black holes: Cosmic history and feedback at the dawn of the universe
topic_facet	Black holes Cosmology Microquasars
description	Significant historic cosmic evolution for the formation rate of stellar black holes is inferred from current theoretical models of the evolution of massive stars, the multiple observations of compact stellar remnants in the near and distant universe, and the cosmic chemical evolution. The mean mass of stellar black holes, the fraction of black holes/neutron stars, and the fraction of black hole high mass X-ray binaries (BH-HMXBs)/solitary black holes increase with redshift. The energetic feedback from large populations of BH-HMXBs form in the first generations of star burst galaxies has been overlooked in most cosmological models of the reionization epoch of the universe. The powerful radiation, jets, and winds from BH-HMXBs heat the intergalactic medium over large volumes of space and keep it ionized until AGN take over. It is concluded that stellar black holes constrained the properties of the faintest galaxies at high redshifts. I present here the theoretical and observational grounds for the historic cosmic evolution of stellar black holes. Detailed calculations on their cosmic impact are presented elsewhere (Mirabel, Dijkstra, Laurent, Loeb, & Pritchard 2011). © International Astronomical Union 2011.
format	SER
author	Mirabel, I.F. Romero G.E. Sunyaev R.A. Sunyaev R.A. Belloni T.M.
author_facet	Mirabel, I.F. Romero G.E. Sunyaev R.A. Sunyaev R.A. Belloni T.M.
author_sort	Mirabel, I.F.
title	Stellar black holes: Cosmic history and feedback at the dawn of the universe
title_short	Stellar black holes: Cosmic history and feedback at the dawn of the universe
title_full	Stellar black holes: Cosmic history and feedback at the dawn of the universe
title_fullStr	Stellar black holes: Cosmic history and feedback at the dawn of the universe
title_full_unstemmed	Stellar black holes: Cosmic history and feedback at the dawn of the universe
title_sort	stellar black holes: cosmic history and feedback at the dawn of the universe
url	http://hdl.handle.net/20.500.12110/paper_17439213_v6_nS275_p3_Mirabel
work_keys_str_mv	AT mirabelif stellarblackholescosmichistoryandfeedbackatthedawnoftheuniverse AT romeroge stellarblackholescosmichistoryandfeedbackatthedawnoftheuniverse AT sunyaevra stellarblackholescosmichistoryandfeedbackatthedawnoftheuniverse AT sunyaevra stellarblackholescosmichistoryandfeedbackatthedawnoftheuniverse AT bellonitm stellarblackholescosmichistoryandfeedbackatthedawnoftheuniverse
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Stellar black holes: Cosmic history and feedback at the dawn of the universe

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