Published in
American Astronomical Society, Astrophysical Journal Supplement, (62), p. 461, 1986
DOI: 10.1086/191148
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A versatile method for obtaining structures of rapidly rotating stars. II - Three-dimensional self-consistent field method
Journal article published in 1986 by
Izumi Hachisu 
This paper was not found in any repository, but could be made available legally by the author.
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