Statistics – Computation
Scientific paper
Dec 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.162...13u&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 162, no. 1, Dec. 1989, p. 13-25.
Statistics
Computation
6
Chemical Composition, Computational Astrophysics, Stellar Cores, Stellar Mass, Stellar Models, Convection, Gravitational Effects, Helium, Mixing Length Flow Theory, Temperature Gradients
Scientific paper
Some problems in constructing the massive star models which have a chemically-inhomogeneous convective core by using the local mixing-length theory are indicated. One problem is negative helium flux. Another one is a large discontinuity in velocity in the convective region. It does not seem easy to reconcile these problems with the present local mixing-length theory.
No associations
LandOfFree
Some problems in constructing massive star models containing a chemically-inhomogeneous convective core with the local mixing-length theory does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Some problems in constructing massive star models containing a chemically-inhomogeneous convective core with the local mixing-length theory, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Some problems in constructing massive star models containing a chemically-inhomogeneous convective core with the local mixing-length theory will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1566827