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- W2078341390 abstract "The formation and evolution of low-mass X-ray binaries (LMXBs) is not well understood. The properties of a population of LMXBs depend on a number of uncertain aspects of binary evolution, and population studies offers a relatively new way of probing binary interactions. We have studied the shape of the faint end of the X-ray luminosity function (LF) of LMXBs in nearby galaxies with Chandra and in the Milky Way using the Swift all-sky monitor. We find a clear difference between the LF of LMXBs in globular clusters (GCs) and those outside, with a relative lack of faint GC sources. This indicates a difference in the composition of the two populations." @default.
- W2078341390 created "2016-06-24" @default.
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- W2078341390 date "2010-01-01" @default.
- W2078341390 modified "2023-09-23" @default.
- W2078341390 title "Binary Evolution Constraints from Luminosity Functions of LMXBs" @default.
- W2078341390 doi "https://doi.org/10.1063/1.3536396" @default.
- W2078341390 hasPublicationYear "2010" @default.
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