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Observational constraints on massive binaries
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Binary interactions are commonplace among massive stars, giving rise observed phenomena such as X-ray binaries, stripped stars & supernovae, and gravitational-wave sources. The multiplicity properties of massive stars thus represent a fundamental observable to calibrate, test, and benchmark models of single-star and binary evolution. In these proceedings, I provide a modern summary of the observed properties of massive binaries across various metallicities, and discuss open problems in the field.
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Cited by 1 Pith paper
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The Samples and Binary Fractions of Red Supergiant in M31 and M33 by the HST Observations
About 31-33% of red supergiants in M31 and M33 show ultraviolet excess from hot companions, giving new HST-based binary fractions.
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