The ubiquity of the rms–flux relation in black hole X-ray binaries
Low- and intermediate-mass close binary evolution and the initial-final mass relation
Period–luminosity relation for persistent low‐mass X‐ray binaries in the near‐infrared
Low- and intermediate-mass close binary evolution and the initial–final mass relation – II. Non-conservative case with convective overshooting
Hard-tail emission in the soft state of low-mass X-ray binaries and their relation to the neutron star magnetic field
Application of the Ghosh & Lamb relation to the spin-up/down behavior in the X-ray binary pulsar 4U 1626−67
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A relation defined between two sets.
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