Core Formation
Core Formation is a planetary differentiation process in which dense, typically metallic (iron‑nickel–rich) material segregates from a partially or fully molten silicate body and sinks gravitationally toward its center to establish a distinct central core.
1.6K
Publications
110.6K
Citations
3.6K
Authors
1.1K
Institutions
Publications per year
2017–2026
294
1.6K
Theory of core-collapse supernovae
Hans‐Thomas Janka, K. Langanke, Alexander Marek et al. · Physics Reports · 2007 · 895 citations · Full text
Natural Sciences, Astronomy, Physics +10
Nucleosynthesis in Supernovae.
F. Hoyle, William A. Fowler · The Astrophysical Journal · 1960 · 835 citations
1–5 of 1.6K
3.6K
24
h-index
22
h-index
21
h-index
19
h-index
19
h-index
1–5 of 3.6K
1.1K

Centre National de la Recherche Scientifique
Paris, France
58 h-index
387 publications
24.7K citations
Planetary Science Institute
Tucson, United States
55 h-index
189 publications
24.3K citations

Carnegie Institution for Science
Washington, United States
46 h-index
170 publications
16.7K citations

Institut de physique du globe de Paris
Paris, France
41 h-index
151 publications
11.9K citations
California Institute of Technology
Pasadena, United States
38 h-index
88 publications
6.7K citations
Geophysical Laboratory
Washington, United States
37 h-index
117 publications
13K citations
University of Bayreuth
Bayreuth, Germany
35 h-index
128 publications
14.6K citations
University of California, Berkeley
Berkeley, United States
34 h-index
81 publications
7.1K citations
1–8 of 1.1K
95 publications · 15.8K citations
70
h-index
161 publications · 12.1K citations
65
h-index
93 publications · 7.4K citations
54
h-index
52 publications · 7.8K citations
44
h-index
ApJ · 72 publications · 6.4K citations
43
h-index
1–5