2-dimensional models of rapidly rotating stars I. Uniformly rotating zero age main sequence stars

DOI10.1051/0004-6361:20041202zbMath1065.85006OpenAlexW2146924433WikidataQ68848739 ScholiaQ68848739MaRDI QIDQ4658926

Ian W. Roxburgh

Publication date: 21 March 2005

Published in: Astronomy & Astrophysics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1051/0004-6361:20041202

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15)

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