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- W2766055867 abstract "We investigate the lack of observed low-mass black hole binary systems at short periods(<4 h) by comparing the observed orbital period distribution of 17 confirmed low-mass black hole X-ray binaries (BHXBs) with their implied period distribution after correcting for the effects of extinction of the optical counterpart, absorption of the X-ray outburst and the probability of detecting a source in outburst. We also draw samples from two simple orbital period distributions and compare the simulated and observed orbital period distributions. We predict that there are >200 and <3000 binaries in the Galaxy with periods between 2 and 3 h, with an additional ≈600 objects between 3 and 10 h." @default.
- W2766055867 created "2017-11-10" @default.
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- W2766055867 date "2017-10-25" @default.
- W2766055867 modified "2023-10-04" @default.
- W2766055867 title "Selection effects on the orbital period distribution of low-mass black hole X-ray binaries" @default.
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- W2766055867 doi "https://doi.org/10.1093/mnras/stx2762" @default.
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