Differential rotation and polar hollows

Details Differential rotation and polar hollows Differential rotation and polar hollows

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992mnras.257..340s&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 257, no. 2, July 15, 1992, p. 340-352. Research support

Statistics

Computation

2

Stellar Rotation, Stellar Structure, Computational Astrophysics, Shapes, Stellar Models

Scientific paper

The notion that differentially rotating stars develop hollows in their polar regions if the differential rotation is sufficiently extreme is quantified, and the sometimes bizarre shapes of stars over a large range of differential rotation and rotation speed are explored. Ranges in which there are no physical solutions are found, but it is argued that some stable single stars with hollows may exist.

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