Bulge-disk Decomposition
Bulge-Disk Decomposition is a quantitative image analysis method in galaxy morphology that separates a galaxy’s light distribution into structurally distinct components—specifically a centrally concentrated bulge and an extended disk—by fitting two-dimensional surface brightness profiles to distinguish their photometric and structural properties.
284
Publications
22.8K
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851
Authors
370
Institutions
Publications per year
2017–2026
66
Variants
Bulge-to-disk DecompositionBulge/disk Decomposition
284
The nuclear bulge of the Galaxy
R. Launhardt, R. Zylka, P. G. Mezger · Astronomy and Astrophysics · 2002 · 474 citations · Full text
Natural Sciences, Astronomy, Physics +17
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Space Telescope Science Institute
Baltimore, United States
25 h-index
55 publications
5K citations
University of California, Santa Cruz
Santa Cruz, United States
22 h-index
90 publications
9.9K citations
European Southern Observatory
Santiago, Chile
21 h-index
27 publications
2.4K citations
Instituto de Astrofísica de Canarias
Tenerife, Spain
21 h-index
67 publications
4.2K citations
Max Planck Institute for Extraterrestrial Physics
Garching bei München, Germany
19 h-index
43 publications
5.7K citations
Swinburne University of Technology
Melbourne, Australia
19 h-index
30 publications
2.1K citations

University of Nottingham
Nottingham, United Kingdom
18 h-index
40 publications
2.3K citations

Universidad de La Laguna
San Cristóbal de La Laguna, Spain
16 h-index
47 publications
2.2K citations
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78 publications · 6.3K citations
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ApJ · 64 publications · 5.5K citations
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AJ · 27 publications · 1.9K citations
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29 publications · 1.5K citations
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19 publications · 3.3K citations
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