Differential rotation along the lower main sequence - A theoretical investigation

Details Differential rotation along the lower main sequence - A theoretical investigation Differential rotation along the lower main sequence - A theoretical investigation

Aug 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....88..240b&link_type=abstract

Astronomy and Astrophysics, vol. 88, no. 1-2, Aug. 1980, p. 240-247. Research supported by the Consiglio Nazionale delle Ricerc

Astronomy and Astrophysics

Astrophysics

30

Convective Flow, Main Sequence Stars, Stellar Atmospheres, Stellar Models, Stellar Rotation, Angular Velocity, Boltzmann Transport Equation, Compressible Flow, Differential Calculus

Scientific paper

The analysis of convection interacting with rotation in a compressible medium is applied to lower main sequence stars. Models of differential rotation were developed for main sequence stars of the types F5, G5, K0, K5, and M0; the rate of differential rotation in latitude at the surface was determined. Results show a definite tendency of differential rotation to decrease from a maximum at F5 to a minimum at G5, and then to increase towards later spectral types.

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