Stellar Radii

Stellar Radii is a metric in astrophysics that quantifies the physical size of stars by measuring the distance from their center to their outermost visible boundary, serving as a fundamental parameter for characterizing stellar structure and evolution.

1.3K

Publications

106.3K

Citations

4.5K

Authors

1K

Institutions

Publications per year

2017–2026

364

Variants

Stellar Radius

Authors

4.5K

  1. DR
    David R. Ciardi

    California Institute of Technology, United States

    21 publications · 2.8K citations

    19

    h-index

  2. DQ
    D. Queloz

    University of Geneva, Switzerland

    22 publications · 1.2K citations

    18

    h-index

  3. DH
    Daniel Huber

    Aarhus University, Denmark

    19 publications · 2.5K citations

    17

    h-index

  4. AW
    Andrew W. Howard

    University of California, Berkeley, United States

    19 publications · 2.8K citations

    17

    h-index

  5. DW
    David W. Latham

    Center for Astrophysics Harvard & Smithsonian, United States

    20 publications · 3.3K citations

    17

    h-index

1–5 of 4.5K

Venues

  1. The Astrophysical Journal

    ApJ · 399 publications · 39.5K citations

    102

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    211 publications · 11.9K citations

    62

    h-index

  3. Astronomy and Astrophysics

    168 publications · 11.1K citations

    57

    h-index

  4. The Astronomical Journal

    AJ · 134 publications · 10K citations

    55

    h-index

  5. The Astrophysical Journal Letters

    40 publications · 3.5K citations

    33

    h-index

1–5