Circulation in AM star envelopes

Details Circulation in AM star envelopes Circulation in AM star envelopes

Sep 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979a%26a....78..119m&link_type=abstract

Astronomy and Astrophysics, vol. 78, no. 1, Sept. 1979, p. 119-121.

Astronomy and Astrophysics

Astrophysics

7

A Stars, Atmospheric Circulation, Magnetic Stars, Stellar Atmospheres, Stellar Envelopes, Angular Momentum, Angular Velocity, Atmospheric Diffusion, Helium, Meridional Flow, Molecular Weight

Scientific paper

In the context of the theory advanced by Vauclair to explain the Am star phenomenum, two additional effects are briefly discussed. These are the choking of the meridional circulation near the stellar surface by the gradient of molecular weight produced by the downward diffusion of helium; and the enhanced value of the rotationally driven circulation found in 2nd order theory.

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