Astronomy and Astrophysics – Astrophysics
Scientific paper
Sep 1969
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969ap%26ss...5...71a&link_type=abstract
Astrophysics and Space Science, Volume 5, Issue 1, pp.71-75
Astronomy and Astrophysics
Astrophysics
1
Scientific paper
Boundary conditions are imposed upon the solutions of the conservation equations for non-thermal convective motion in a self-gravitating, homogeneous, non-rotating sphere of radiusR, consisting of a core extending to a fraction η of the radius of the sphere and with a viscous mantle overlying the core. It is shown that convective modes are permissible in the mantle only for certain values ofn and η.
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