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- W2077874 abstract "Abstract Using the maximum likelihood method we show that the observed distribution of maximum frequencies of kilohertz quasi periodic oscillations (QPOs) in LMXBs agrees with the frequencies of orbital motion in the marginally stable orbit around compact objects with masses chosen randomly from some interval, which we find to be (1.55 M ⊙ , 2.40 M ⊙ ) at the 99% confidence level. As this remarkable agreement with the expected mass range of neutron stars in LMXBs demonstrates, the assumption that the maximum-frequency QPOs occur in the marginally stable orbit is consistent with the current data set." @default.
- W2077874 created "2016-06-24" @default.
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- W2077874 date "2000-01-01" @default.
- W2077874 modified "2023-09-27" @default.
- W2077874 title "Kilohertz QPOs and general-relativistic orbital motion—a maximum likelihood test" @default.
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- W2077874 doi "https://doi.org/10.1017/s0252921100060887" @default.
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