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Models for highly flattened, rapidly rotating cool stars in a Newtonian approximation

✍ Scribed by D. P. Savokhin; E. I. Saritsin; S. I. Blinnikov


Book ID
110127828
Publisher
Springer
Year
2001
Tongue
English
Weight
122 KB
Volume
45
Category
Article
ISSN
1063-7729

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