Third Dredge-up
Third Dredge-Up is a stellar nucleosynthetic process in asymptotic giant branch stars whereby partially processed material from the helium-burning shell is transported to the outer envelope via convective mixing following a thermal pulse, thereby altering the surface composition through the enrichment of carbon and s-process elements.
117
Publications
13.4K
Citations
213
Authors
136
Institutions
Publications per year
2017–2026
18
Parents
117
1–5 of 117
213
14
h-index
11
h-index
11
h-index
10
h-index
7
h-index
1–5 of 213
136
Collurania Teramo Observatory
Teramo, Italy
18 h-index
32 publications
7.8K citations

Monash University
Melbourne, Australia
17 h-index
38 publications
4.6K citations
University of Vienna
Vienna, Austria
12 h-index
19 publications
1.4K citations

University of Turin
Turin, Italy
12 h-index
19 publications
9.3K citations
Osservatorio Astronomico di Padova
Padua, Italy
11 h-index
22 publications
2.8K citations
Université Libre de Bruxelles
Brussels, Belgium
11 h-index
32 publications
1.6K citations
KU Leuven
Leuven, Belgium
8 h-index
16 publications
452 citations
Institute of Astronomy
Moscow, Russia
7 h-index
15 publications
639 citations
1–8 of 136
ApJ · 26 publications · 3.9K citations
25
h-index
27 publications · 1.6K citations
22
h-index
23 publications · 2.8K citations
20
h-index
Repository · 5 publications · 70 citations
5
h-index
4 publications · 1.2K citations
4
h-index
1–5