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- W3100481448 abstract "Aims. We model the present-day population of classical low-mass X-ray binaries (LMXBs) with neutron star accretors, which have hydrogen-rich donor stars. Their population is compared with that of hydrogen-deficient LMXBs, known as ultracompact X-ray binaries (UCXBs). We model the observable LMXB population and compare it to observations. We model the Galactic Bulge because it contains a well-observed population and it is the target of the Galactic Bulge Survey." @default.
- W3100481448 created "2020-11-23" @default.
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- W3100481448 date "2015-06-23" @default.
- W3100481448 modified "2023-10-10" @default.
- W3100481448 title "Population synthesis of classical low-mass X-ray binaries in the Galactic Bulge" @default.
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- W3100481448 doi "https://doi.org/10.1051/0004-6361/201425303" @default.
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