REVIEW 2 cited by
Stellar evolution of low and intermediate-mass stars. IV. Hydrodynamically-based overshoot and nucleosynthesis in AGB stars
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
read the original abstract
The focus of this study is on the treatment of those stellar regions immediately adjacent to convective zones. The results of hydrodynamical simulations by Freytag et al. (1996, A&A313,497) show that the motion of convective elements extends well beyond the boundary of the convectively unstable region. We have applied their parametrized description of the corresponding velocities to the treatment of overshoot in stellar evolution calculations up to the AGB (Pop.I, M_zams=3M_sun).
Forward citations
Cited by 2 Pith papers
-
The s- and r- components of the proto-solar composition
Overview of methods and recent developments for deriving s- and r-process components of the proto-solar composition.
-
Evolution and final fates of massive stars
A review chapter condensing standard models and open uncertainties in the evolution and final fates of massive stars.
Discussion (0). Continue with ORCID to comment.