Astronomy and Astrophysics – Astrophysics
Scientific paper
2007-09-03
Astronomy and Astrophysics
Astrophysics
Invited conference paper given at "Why Galaxies Care About AGB Stars", Vienna, August 7-11, 2006, to appear in ASP Conference
Scientific paper
We review the current state of modeling convective mixing in AGB stars. The focus is on results obtained through multi-dimensional hydrodynamic simulations of AGB convection, both in the envelope and the unstable He-shell. Using two different codes and a wide range of resolutions and modeling assumptions we find that mixing across convective boundaries is significant for He-shell flash convection. We present a preliminary quantitative analysis of this convectively induced extra mixing, based on a sub-set of our simulations. Other non-standard mixing will be discussed briefly.
Freytag Bernd
Fuchs Tyler
Hansen James P.
Herwig Falk
Hueckstaedt Robert M.
No associations
LandOfFree
Convective and non-convective mixing in AGB stars 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 Convective and non-convective mixing in AGB stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Convective and non-convective mixing in AGB stars will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-468081