Stellar Metallicities
Stellar Metallicities is a quantitative astrophysical construct that measures the abundance fraction of chemical elements heavier than helium in a star relative to hydrogen, serving as a key diagnostic for stellar nucleosynthetic history and galactic chemical evolution.
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Carlos A. Iglesias, F. J. Rogers · The Astrophysical Journal · 1996 · 3K citations
Natural Sciences, Astronomy, Physics +14
THE OBSERVED PROPERTIES OF DWARF GALAXIES IN AND AROUND THE LOCAL GROUP
The Astronomical Journal · 2012 · 1.9K citations · Full text
Natural Sciences, Astronomy, Physics +16
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Centre National de la Recherche Scientifique
Paris, France
101 h-index
1.7K publications
148.3K citations
The University of Texas at Austin
Austin, United States
95 h-index
416 publications
44.3K citations
Osservatorio Astronomico di Padova
Padua, Italy
95 h-index
604 publications
97.2K citations
California Institute of Technology
Pasadena, United States
93 h-index
423 publications
53.5K citations
University of Cambridge
Cambridge, United Kingdom
92 h-index
559 publications
57.3K citations

Australian National University
Canberra, Australia
91 h-index
703 publications
59.1K citations
Carnegie Observatories
Pasadena, United States
87 h-index
356 publications
38.9K citations
Instituto de Astrofísica de Canarias
Tenerife, Spain
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735 publications
88.7K citations
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ApJ · 1.5K publications · 138.4K citations
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AJ · 420 publications · 40.4K citations
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