Nebular Metallicity
Nebular Metallicity is the measure of the abundance of chemical elements heavier than helium in ionized gas regions of interstellar space, relative to hydrogen, used as an indicator of galactic chemical evolution and star formation history.
339
Publications
24.9K
Citations
1.3K
Authors
464
Institutions
Publications per year
2017–2026
79
Parents
339
An abundance of small exoplanets around stars with a wide range of metallicities
Lars A. Buchhave, David W. Latham, Anders Johansen et al. · Nature · 2012 · 740 citations
Natural Sciences, Astronomy, Physics +14
Nebular emission from star-forming galaxies
S. Charlot, M. Longhetti · Monthly Notices of the Royal Astronomical Society · 2001 · 481 citations · Full text
Natural Sciences, Astronomy, Physics +17
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Centre National de la Recherche Scientifique
Paris, France
31 h-index
90 publications
7.5K citations
University of Cambridge
Cambridge, United Kingdom
25 h-index
64 publications
4.8K citations

Space Telescope Science Institute
Baltimore, United States
21 h-index
49 publications
2.9K citations
California Institute of Technology
Pasadena, United States
20 h-index
55 publications
5.3K citations
European Southern Observatory
Garching bei München, Germany
18 h-index
31 publications
1.5K citations
Institut d'Astrophysique de Paris
Paris, France
17 h-index
31 publications
4.1K citations
University of California, Los Angeles
Los Angeles, United States
16 h-index
25 publications
1.5K citations
Universidad Nacional Autónoma de México
Mexico City, Mexico
16 h-index
23 publications
1.6K citations
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ApJ · 96 publications · 9.5K citations
54
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85 publications · 6.9K citations
45
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38 publications · 2.4K citations
28
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AJ · 15 publications · 882 citations
14
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9 publications · 362 citations
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