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Black hole high mass X-ray binary microquasars at cosmic dawn

Published online by Cambridge University Press:  30 December 2019

I. F. Mirabel
I. F. Mirabel*
Affiliation:
Institute of Astronomy and Space Physics. CONICET - Universidad de Buenos Aires, Ciudad Universitaria, Av. Cantilo S/N, 1428 Buenos Aires - Argentina Laboratoire AIM-Paris-Saclay, CEA/DSM/Irfu/DAPâ^’CNRS, CEA-Saclay, pt courrier 131, 91191 Gif-sur-Yvette, France
*
email: mirabel@iafe.uba.ar
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Abstract

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Theoretical models and observations suggest that primordial Stellar Black Holes (Pop-III-BHs) were prolifically formed in HMXBs, which are powerful relativistic jet sources of synchrotron radiation called Microquasars (MQs).

Large populations of BH-HMXB-MQs at cosmic dawn produce a smooth synchrotron cosmic radio background (CRB) that could account for the excess amplitude of atomic hydrogen absorption at z∼17, recently reported by EDGES.

BH-HMXB-MQs at cosmic dawn precede supernovae, neutron stars and dust. BH-HMXB-MQs promptly inject into the IGM hard X-rays and relativistic jets, which overtake the slowly expanding HII regions ionized by progenitor Pop-III stars, heating and partially ionizing the IGM over larger distance scales.

BH-HMXBs are channels for the formation of Binary-Black-Holes (BBHs). The large masses of BBHs detected by gravitational waves, relative to the masses of BHs detected by X-rays, and the high rates of BBH-mergers, are consistent with high formation rates of BH-HMXBs and BBHs in the early universe.

Keywords

X-rays: binariesmicroquasarsearly universe(cosmology:) black hole physicsgravitational waves
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S346: High-mass X-ray Binaries: Illuminating the Passage from Massive Binaries to Merging Compact Objects , August 2018 , pp. 365 - 379
Copyright
© International Astronomical Union 2019 

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