Astronomy and Astrophysics – Astrophysics
Scientific paper
2002-08-14
Mon.Not.Roy.Astron.Soc.339:515,2003
Astronomy and Astrophysics
Astrophysics
10 pages, 11 figures, 5 tables, submitted to MNRAS
Scientific paper
10.1046/j.1365-8711.2003.06190.x
We give a thorough investigation of sequences of uniformly rotating, homogeneous axisymmetric Newtonian equilibrium configurations that bifurcate from highly flattened Maclaurin spheroids. Each one of these sequences possesses a mass-shedding limit. Starting at this point, the sequences proceed towards the Maclaurin sequence and beyond. The first sequence leads to the well known Dyson rings, whereas the end points of the higher sequences are characterized by the formation of a two-body system, either a core-ring system (for the second, the fourth etc. sequence) or a two-ring system (for the third, the fifth etc. sequence). Although the general qualitative picture drawn by Eriguchi and Hachisu in the eighties has been confirmed, slight differences turned out in the interpretation of the origin of the first two-ring sequence and in the general appearance of fluid bodies belonging to higher sequences.
Ansorg Marcus
Kleinwächter Andreas
Meinel Reinhard
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