Lithium Abundance

Lithium Abundundance is a quantitative astrophysical measure representing the relative number density of lithium atoms in a stellar atmosphere, distinguished by its sensitivity to stellar evolutionary phase and use as a diagnostic tracer of mixing processes and age in low-mass and pre-main sequence stars.

1.2K

Publications

71.3K

Citations

2.9K

Authors

945

Institutions

Publications per year

2017–2026

197

Authors

2.9K

  1. CP
    Constantine P. Deliyannis

    Indiana University Bloomington, United States

    34 publications · 2.4K citations

    28

    h-index

  2. DL
    David L. Lambert

    The University of Texas at Austin, United States

    29 publications · 2.4K citations

    25

    h-index

  3. SR
    S. Randich

    Arcetri Astrophysical Observatory, Italy

    27 publications · 1.4K citations

    23

    h-index

  4. PB
    P. Bonifacio

    Galaxies, Etoiles, Physique et Instrumentation, France

    27 publications · 2.3K citations

    22

    h-index

  5. AM
    Ann Merchant Boesgaard

    University of Hawaiʻi at Mānoa, United States

    26 publications · 1.8K citations

    22

    h-index

1–5 of 2.9K

Venues

  1. The Astrophysical Journal

    ApJ · 244 publications · 16.6K citations

    75

    h-index

  2. Astronomy and Astrophysics

    163 publications · 9.3K citations

    54

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    86 publications · 4.3K citations

    36

    h-index

  4. The Astronomical Journal

    AJ · 49 publications · 3.9K citations

    33

    h-index

  5. Geochimica et Cosmochimica Acta

    36 publications · 3.7K citations

    30

    h-index

1–5