Rotational Broadening

Rotational Broadening is a spectroscopic phenomenon in stellar astronomy whereby the spectral lines of a rotating star are widened due to the Doppler shifts arising from the differential line-of-sight velocities across the star’s rotating surface.

276

Publications

14.1K

Citations

906

Authors

376

Institutions

Publications per year

2017–2026

46

Authors

906

  1. AS
    A. Sozzetti

    Osservatorio Astrofisico di Torino, Italy

    27 publications · 781 citations

    18

    h-index

  2. FB
    F. Borsa

    Brera Astronomical Observatory, Italy

    23 publications · 720 citations

    17

    h-index

  3. AF
    A. F. Lanza

    Osservatorio Astrofisico di Catania, Italy

    26 publications · 730 citations

    17

    h-index

  4. AS
    A. S. Bonomo

    Osservatorio Astrofisico di Torino, Italy

    25 publications · 740 citations

    17

    h-index

  5. AB
    A. Bignamini

    Trieste Astronomical Observatory, Italy

    25 publications · 744 citations

    17

    h-index

1–5 of 906

Venues

  1. The Astrophysical Journal

    ApJ · 75 publications · 4K citations

    37

    h-index

  2. Astronomy and Astrophysics

    52 publications · 2.5K citations

    26

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    27 publications · 1.7K citations

    22

    h-index

  4. The Journal of Chemical Physics

    15 publications · 969 citations

    14

    h-index

  5. The Astronomical Journal

    AJ · 15 publications · 1.3K citations

    14

    h-index

1–5