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Dynamics of stellar black holes in young star clusters with different metallicities - I. Implications for X-ray binaries

Monthly Notices of the Royal Astronomical Society, no. 3 (2013): 2298-2314

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academic.microsoft.com arxiv.org

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black hole physicsmethods: numericalbinaries: generalstars: kinematics and dynamicsgalaxies: star clusters: general更多(1+)

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We present N-body simulations of intermediate-mass (3000–4000 M⊙) young star clusters (SCs) with three different metallicities (Z = 0.01, 0.1 and 1 Z⊙), including metal-dependent stellar evolution recipes and binary evolution. Following recent theoretical models of wind mass-loss and core-collapse supernovae, we assume that the mass of th...更多

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