Stellar Streams

Stellar Streams is a stellar kinematic structure consisting of elongated, coherent trails of stars that originate from tidally disrupted star clusters, dwarf galaxies, or stellar associations and that orbit within the galactic halo, serving as tracers of the gravitational potential and hierarchical assembly history of the Milky Way.

558

Publications

41K

Citations

1.2K

Authors

478

Institutions

Publications per year

2017–2026

226

Authors

1.2K

  1. RI
    Rodrigo Ibata

    Observatoire astronomique de Strasbourg, France

    37 publications · 3.3K citations

    28

    h-index

  2. VB
    Vasily Belokurov

    University of Cambridge, United Kingdom

    33 publications · 4.5K citations

    28

    h-index

  3. DE
    Denis Erkal

    University of Surrey, United Kingdom

    28 publications · 2.7K citations

    25

    h-index

  4. SE
    S. E. Koposov

    University of Cambridge, United Kingdom

    25 publications · 2.2K citations

    22

    h-index

  5. GF
    Geraint F. Lewis

    The University of Sydney, Australia

    23 publications · 2.7K citations

    22

    h-index

1–5 of 1.2K

Venues

  1. The Astrophysical Journal

    ApJ · 166 publications · 17.2K citations

    67

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    151 publications · 10.3K citations

    56

    h-index

  3. Astronomy and Astrophysics

    50 publications · 2.5K citations

    31

    h-index

  4. The Astrophysical Journal Letters

    29 publications · 1.7K citations

    25

    h-index

  5. The Astronomical Journal

    AJ · 31 publications · 2K citations

    21

    h-index

1–5