Black hole/pulsar binaries in the Galaxy. (18th April 2018)

• Record Type: Journal Article
• Authors: Shao, Yong; Li, Xiang-Dong
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 477:Number 1(2018:Jun.)
• Page Start: L128
• Page End: L132
• Publication Date: 2018-04-18
• Subjects: binaries: general -- stars: neutron -- stars: black holes; Astronomy -- Research -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnrasl/sly063
• Languages: English
• ISSNs: 1745-3933

Abstract

ABSTRACT: We have performed population synthesis calculation on the formation of binaries containing a black hole (BH) and a neutron star (NS) in the Galactic disc. Some of important input parameters, especially for the treatment of common envelope evolution, are updated in the calculation. We have discussed the uncertainties from the star formation rate of the Galaxy and the velocity distribution of NS kicks on the birthrate (${\sim } 0.6\hbox{--}13 \rm \, M\, yr^{-1}$ ) of BH/NS binaries. From incident BH/NS binaries, by modelling the orbital evolution due to gravitational wave radiation and the NS evolution as radio pulsars, we obtain the distributions of the observable parameters such as the orbital period, eccentricity, and pulse period of the BH/pulsar binaries. We estimate that there may be ∼3–80 BH/pulsar binaries in the Galactic disc and around 10 per cent of them could be detected by the Five-hundred-metre Aperture Spherical radio Telescope.