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- W2036960168 abstract "Abstract Our aim is to investigate tidal interaction in High‐Mass X‐ray Binary stars in order to determine in which objects the rotation of the mass donors is synchronized or pseudosynchronized with the orbital motion of the compact companion. We calculate the pseudosynchronization period ( P ps ) and compare it with the rotational period of the mass donors ( P rot ). We find that (1) the Be/X‐ray binaries are not synchronized, the mass donors rotate faster than the orbital period and the ratio P ps / P rot is 2–300; (2) the giant and supergiant systems are close to synchronization and for them the ratio P ps / P rot is 0.3–2 (© 2009 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)" @default.
- W2036960168 created "2016-06-24" @default.
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- W2036960168 date "2009-07-17" @default.
- W2036960168 modified "2023-10-18" @default.
- W2036960168 title "Tidal interaction in High-Mass X-ray Binaries" @default.
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- W2036960168 doi "https://doi.org/10.1002/asna.200811224" @default.
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