Mass-metallicity Relation
The Mass-Metallicity Relation is an empirical astrophysical correlation that describes the observed trend wherein the gas-phase metallicity of a star-forming galaxy increases with its stellar mass, reflecting the interplay between star formation, chemical enrichment, and galactic-scale feedback processes.
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Mass-metallicity RelationshipMzr
Parents
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Mass-loss predictions for O and B stars as a function of metallicity
Astronomy and Astrophysics · 2001 · 1.7K citations · Full text
Natural Sciences, Astronomy, Physics +17
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Centre National de la Recherche Scientifique
Paris, France
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567 publications
44.2K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
55 h-index
171 publications
17.2K citations

Space Telescope Science Institute
Baltimore, United States
53 h-index
172 publications
13.4K citations
California Institute of Technology
Pasadena, United States
53 h-index
167 publications
25.9K citations
European Southern Observatory
Garching bei München, Germany
51 h-index
166 publications
15.5K citations
University of California, Santa Cruz
Santa Cruz, United States
51 h-index
154 publications
15.6K citations
Instituto de Astrofísica de Canarias
Tenerife, Spain
49 h-index
200 publications
17.5K citations
University of Cambridge
Cambridge, United Kingdom
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188 publications
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ApJ · 517 publications · 52.7K citations
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498 publications · 42.4K citations
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AJ · 113 publications · 9.8K citations
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