Evolution of rotating massive main sequence stars: The role of shear turbulence in the radiative envelope of a 16 Msun star

Details Evolution of rotating massive main sequence stars: The role of shear turbulence in the radiative envelope of a 16 Msun star Evolution of rotating massive main sequence stars: The role of shear turbulence in the radiative envelope of a 16 Msun star

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999arep...43..592s&link_type=abstract

Astronomy Reports, Volume 43, Issue 9, September 1999, pp.592-600

Astronomy and Astrophysics

Astronomy

3

Scientific paper

Shear turbulence in the radiative envelope of a rotating massive
main-sequence star transfers angular momentum from deep inner layers up
to the surface. As a result, the impact of rotation on the radius of the
star increases, causing the main sequence to broaden.

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