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.

3.1K

Publications

186.7K

Citations

7.7K

Authors

1.9K

Institutions

Publications per year

2017–2026

588

Authors

7.7K

  1. TC
    Timothy C. Beers

    Michigan State University, United States

    79 publications · 11.3K citations

    54

    h-index

  2. MA
    M. Asplund

    Australian National University, Australia

    71 publications · 10.1K citations

    50

    h-index

  3. DL
    David L. Lambert

    The University of Texas at Austin, United States

    75 publications · 5.9K citations

    41

    h-index

  4. VH
    V. Hill

    Centre National de la Recherche Scientifique, France

    41 publications · 7.6K citations

    38

    h-index

  5. WA
    Wako Aoki

    National Astronomical Observatory of Japan, Japan

    53 publications · 4.9K citations

    38

    h-index

1–5 of 7.7K

Venues

  1. The Astrophysical Journal

    ApJ · 598 publications · 46.3K citations

    103

    h-index

  2. Astronomy and Astrophysics

    436 publications · 34.1K citations

    97

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    305 publications · 16.9K citations

    62

    h-index

  4. The Astronomical Journal

    AJ · 135 publications · 11.2K citations

    58

    h-index

  5. The Astrophysical Journal Supplement Series

    47 publications · 5.5K citations

    32

    h-index

1–5