Multiwavelength detectability of isolated black holes in the Milky Way

被引：8

作者：

Scarcella, Francesca ^{[1
]}

Gaggero, Daniele ^{[1
]}

Connors, Riley ^{[2
]}

Manshanden, Julien ^{[3
]}

Ricotti, Massimo ^{[4
]}

Bertone, Gianfranco ^{[5
,6
]}

机构：

[1] UAM, Inst Fis Teor, CSIC, Campus Cantoblanco, E-28049 Madrid, Spain

[2] CALTECH, Cahill Ctr Astron & Astrophys, Pasadena, CA 91125 USA

[3] Univ Hamburg, Inst Theores Phys 2, D-22761 Hamburg, Germany

[4] Univ Maryland, Dept Astron, College Pk, MD 20740 USA

[5] Univ Amsterdam, Gravitat Astroparticle Phys Amsterdam GRAPPA, Inst Theoret Phys Amsteniam, Sci Pk 904, NL-1098 XH Amsterdam, Netherlands

[6] Univ Amsterdam, Delta Inst Theoret Phys, Sci Pk 904, NL-1098 XH Amsterdam, Netherlands

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2021年 / 505卷 / 03期

关键词：

astroparticle physics; black hole physics; ISM: jets and outflows; X-RAY BINARIES; ADVECTION-DOMINATED ACCRETION; RADIO-EMISSION; FUNDAMENTAL PLANE; LOW/HARD STATE; KINEMATICS; EVOLUTION; GALAXIES; JETS; FLOW;

D O I：

10.1093/mnras/stab1533

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Isolated black holes in our Galaxy have eluded detection so far. We present here a comprehensive study on the detectability of isolated stellar-mass astrophysical black holes that accrete interstellar gas from molecular clouds in both the local region and the Central Molecular Zone. We adopt a state-of-the-art model for the accretion physics backed up by numerical simulations, and study the number of observable sources in both the radio and X-ray band, as a function of a variety of parameters. We discuss in particular the impact of the astrophysical uncertainties on our prediction for the number of bright X-ray sources in the central region of the Galaxy. We finally consider future developments in the radio domain and assess the potential of SKA to detect a population of astrophysical black holes accreting gas in our Galaxy.

引用

页码：4036 / 4047

页数：12

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