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- W4387600516 abstract "Abstract When a compact object is formed, an impulse (kick) will be imparted to the system by the mass lost during the core-collapse supernova (SN). A number of other mechanisms may impart an additional kick on the system, although evidence for these natal kicks in black hole systems remains limited. Updated Gaia astrometry has recently identified a number of high peculiar velocity (in excess of Galactic motion) compact objects. Here, we focus on the black hole low-mass X-ray binary H 1705–250, which has a peculiar velocity $upsilon _{mathrm{pec}}, =, 221^{+101}_{-108}, mathrm{km}, mathrm{s}^{-1}$. Using population synthesis to reconstruct its evolutionary history (assuming formation via isolated binary evolution within the Galactic plane), we constrain the properties of the progenitor and pre-SN orbit. The magnitude of a kick solely due to mass loss is found to be ∼ 30 km s−1, which cannot account for the high present-day peculiar motion. We therefore deduce that the black hole received an additional natal kick at formation, and place limits on its magnitude, finding it to be ∼ 295 km s−1 (minimum 90 km s−1). This furthers the argument that these kicks are not limited to neutron stars." @default.
- W4387600516 created "2023-10-14" @default.
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- W4387600516 date "2023-10-13" @default.
- W4387600516 modified "2023-10-14" @default.
- W4387600516 title "On the natal kick of the black hole X-ray binary H 1705–250" @default.
- W4387600516 doi "https://doi.org/10.1093/mnrasl/slad151" @default.
- W4387600516 hasPublicationYear "2023" @default.
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