The interaction of multiple convection zones in A-type stars
A-type stars have a complex internal structure with the possibility of multiple convection zones. If not sufficiently separated, such zones will interact through the convectively stable regions that lie between them. It is therefore of interest to ask whether the typical conditions that exist within...
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Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 2007-09, Vol.380 (1), p.44-50 |
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Sprache: | eng |
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