Elemental Abundance Analysis
Elemental Abundance Analysis is a methodological framework in stellar spectroscopy that quantifies the relative concentrations of chemical elements in a star by interpreting the strengths and patterns of absorption lines in its spectrum, distinguishing it from broader observational techniques through its specific focus on deriving precise compositional data from spectral features.
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Solar System Abundances and Condensation Temperatures of the Elements
K. Lodders · The Astrophysical Journal · 2003 · 4.8K citations · Full text
First stars V - Abundance patterns from C to Zn and supernova yields in the early Galaxy
R. Cayrel, É. Depagne, M. Spite et al. · Astronomy and Astrophysics · 2004 · 1.2K citations · Full text
Natural Sciences, Astronomy, Physics +11
The nitrogen abundance of the very metal-poor star HD 122563.
C. Sneden · The Astrophysical Journal · 1973 · 898 citations
Natural Sciences, Astronomy, Physics +13
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The University of Texas at Austin
Austin, United States
74 h-index
322 publications
31.7K citations

Australian National University
Canberra, Australia
70 h-index
369 publications
41.2K citations

Centre National de la Recherche Scientifique
Paris, France
69 h-index
564 publications
47.1K citations
Michigan State University
East Lansing, United States
57 h-index
104 publications
14.5K citations
Galaxies, Etoiles, Physique et Instrumentation
Meudon, France
57 h-index
358 publications
47.3K citations
Carnegie Observatories
Pasadena, United States
55 h-index
154 publications
18K citations
Instituto de Astrofísica de Canarias
Tenerife, Spain
54 h-index
274 publications
23K citations

Uppsala University
Uppsala, Sweden
53 h-index
145 publications
14.9K citations
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ApJ · 598 publications · 46.3K citations
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AJ · 135 publications · 11.2K citations
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