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Angular velocity distribution in a star that is a component of a close binary and has a rapidly rotating core

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Literature Cited

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Authors
  1. V. G. Gorbatskii
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Additional information

A. A. Zhdanov Leningrad State University. Translated from Astrofizika, Vol. 13, No. 3, pp. 485–492, July–September, 1977.

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Gorbatskii, V.G. Angular velocity distribution in a star that is a component of a close binary and has a rapidly rotating core. Astrophysics 13, 272–276 (1977). https://doi.org/10.1007/BF01001222

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  • DOI: https://doi.org/10.1007/BF01001222

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