Bright end of the luminosity function of high-mass X-ray binaries: 
contributions of hard, soft and supersoft sources

Sazonov, S.; Khabibullin, I.

doi:10.1093/mnras/stw3113

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Bright end of the luminosity function of high-mass X-ray binaries: contributions of hard, soft and supersoft sources

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Khabibullin, I.
High Energy Astrophysics, MPI for Astrophysics, Max Planck Society;

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Sazonov, S., & Khabibullin, I. (2017). Bright end of the luminosity function of high-mass X-ray binaries: contributions of hard, soft and supersoft sources. Monthly Notices of the Royal Astronomical Society, 466(1), 1019-1051. doi:10.1093/mnras/stw3113.

引用: https://hdl.handle.net/11858/00-001M-0000-002D-5510-5

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