Horizontal Branch Evolution
Horizontal Branch Evolution is a phase in stellar evolution characterized by the stable helium core burning and hydrogen shell burning in low- to intermediate-mass stars after they ascend the red giant branch and settle on the horizontal branch in the Hertzsprung–Russell diagram.
355
Publications
26K
Citations
709
Authors
357
Institutions
Publications per year
2017–2026
32
Parents
355
The Dartmouth Stellar Evolution Database
The Astrophysical Journal Supplement Series · 2008 · 1.7K citations · Full text
Natural Sciences, Astronomy, Physics +15
A Triple Main Sequence in the Globular Cluster NGC 2808
The Astrophysical Journal · 2007 · 681 citations · Full text
Natural Sciences, Astronomy, Physics +16
A Triple Main Sequence in the Globular Cluster NGC 2808 1
G. Piotto, L. R. Bedin, Jay Anderson et al. · 2013 · 436 citations
Natural Sciences, Astronomy, Physics +16
1–5 of 355
709
25
h-index
17
h-index
16
h-index
14
h-index
14
h-index
1–5 of 709
357
Collurania Teramo Observatory
Teramo, Italy
30 h-index
63 publications
5.8K citations

Astronomical Observatory of Rome
Rome, Italy
27 h-index
99 publications
5.7K citations
Osservatorio Astronomico di Padova
Padua, Italy
25 h-index
80 publications
7.5K citations

Space Telescope Science Institute
Baltimore, United States
23 h-index
45 publications
3.6K citations
National Institute for Astrophysics
Rome, Italy
22 h-index
91 publications
7K citations
Osservatorio astronomico di Bologna
Bologna, Italy
22 h-index
53 publications
5.7K citations

Centre National de la Recherche Scientifique
Paris, France
21 h-index
40 publications
4.2K citations

University of Padua
Padua, Italy
21 h-index
48 publications
5.3K citations
1–8 of 357
ApJ · 102 publications · 7.6K citations
48
h-index
52 publications · 3.1K citations
34
h-index
49 publications · 4.4K citations
28
h-index
AJ · 46 publications · 3.1K citations
27
h-index
15 publications · 603 citations
13
h-index
1–5