Open AccessThe possibility of non-synchronism of convective secondaries in close binary stars
Author(s) -
C. G. Campbell,
J. C. B. Papaloizou
Publication year - 1983
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-8711
pISSN - 0035-8711
DOI - 10.1093/mnras/204.2.433
Subject(s) - physics , synchronism , convection , rotation (mathematics) , astrophysics , binary number , binary star , turbulence , stars , mechanics , classical mechanics , geometry , mathematics , arithmetic , quantum mechanics , voltage
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