Chandrasekhar's perturbation method-oriented theories up to third order for uniformly and differentially-rotating polytropic stars: error- removing techniques
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Publication:909501
DOI10.1007/BF00644180zbMath0694.70006MaRDI QIDQ909501
Publication date: 1986
Published in: Astrophysics and Space Science (Search for Journal in Brave)
Computational methods for problems pertaining to mechanics of particles and systems (70-08) Celestial mechanics (70F15)
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