Tidal Features

Tidal Features is a morphological signature in galaxy structure consisting of low-surface-brightness debris such as streams, shells, or plumes that arise from gravitational interactions and distinguish themselves from primordial galaxy components by their dynamical origin in tidal disruption events.

300

Publications

21.5K

Citations

1.1K

Authors

498

Institutions

Publications per year

2017–2026

72

Authors

1.1K

  1. PD
    Pierre–Alain Duc

    Centre National de la Recherche Scientifique, France

    6 publications · 427 citations

    6

    h-index

  2. DM
    David Martínez‐Delgado

    Instituto de Astrofísica de Canarias, Spain

    6 publications · 756 citations

    6

    h-index

  3. JC
    J. Christopher Mihos

    Case Western Reserve University, United States

    6 publications · 810 citations

    6

    h-index

  4. JC
    Jean‐Charles Cuillandre

    Centre National de la Recherche Scientifique, France

    5 publications · 196 citations

    5

    h-index

  5. CS
    Curtis Struck

    Iowa State University, United States

    5 publications · 396 citations

    5

    h-index

1–5 of 1.1K

Venues

  1. The Astrophysical Journal

    ApJ · 58 publications · 6K citations

    36

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    48 publications · 2.5K citations

    28

    h-index

  3. The Astronomical Journal

    AJ · 27 publications · 3.2K citations

    23

    h-index

  4. Astronomy and Astrophysics

    17 publications · 671 citations

    14

    h-index

  5. The Astrophysical Journal Letters

    6 publications · 352 citations

    6

    h-index

1–5