wdarnett at gmail.com
Sat Jun 9 12:39:28 EDT 2012
3D simulations suggest that the mixing length is not constant (smaller for
thin convection zones for example; see the white dwarf literature and
compare with standard solar models, e.g.), so that a first step would seem
to be an array for values of the alpha.
University of Arizona
-------------- next part --------------
An HTML attachment was scrubbed...
More information about the Mesa-users