Classical Bulge
Classical Bulge is a structural component of a galaxy characterized by a dense, pressure-supported stellar population that exhibits little to no rotational support and forms through rapid, early hierarchical merging processes distinct from secular evolution.
134
Publications
10.7K
Citations
366
Authors
229
Institutions
Publications per year
2017–2026
45
Variants
Classical Galactic Bulge
Parents
134
OUR MILKY WAY AS A PURE-DISK GALAXY—A CHALLENGE FOR GALAXY FORMATION
Juntai Shen, R. Michael Rich, John Kormendy et al. · The Astrophysical Journal Letters · 2010 · 364 citations · Full text
Natural Sciences, Astronomy, Physics +17
1–5 of 134
366
Max Planck Institute for Extraterrestrial Physics, Germany
8 publications · 736 citations
8
h-index
8
h-index
7
h-index
7
h-index
7
h-index
1–5 of 366
229
Max Planck Institute for Extraterrestrial Physics
Garching bei München, Germany
24 h-index
87 publications
7.2K citations

Centre National de la Recherche Scientifique
Paris, France
19 h-index
55 publications
4.2K citations
Max Planck Institute for Astrophysics
Garching, Germany
13 h-index
17 publications
1.9K citations
The University of Texas at Austin
Austin, United States
13 h-index
19 publications
2.2K citations
Instituto de Astrofísica de Canarias
Tenerife, Spain
12 h-index
20 publications
1K citations
Universidad Nacional Autónoma de México
Mexico City, Mexico
11 h-index
16 publications
1K citations
Laboratoire d’Astrophysique de Marseille
Marseille, France
10 h-index
15 publications
1.2K citations

Universidad de La Laguna
San Cristóbal de La Laguna, Spain
10 h-index
16 publications
777 citations
1–8 of 229
52 publications · 3.9K citations
31
h-index
ApJ · 27 publications · 2.4K citations
22
h-index
18 publications · 1.4K citations
17
h-index
10 publications · 904 citations
10
h-index
Repository · 5 publications · 286 citations
5
h-index
1–5