Filamentary Structure

Filamentary Structure is a morphological feature in the interstellar medium characterized by elongated, thread-like configurations of gas and dust that emerge from gravitational instabilities and turbulence in star-forming regions, serving as privileged sites for the formation of dense cores and protostellar systems within the large-scale structure of molecular clouds.

2.8K

Publications

178.8K

Citations

8.7K

Authors

1.8K

Institutions

Publications per year

2017–2026

619

Authors

8.7K

  1. DW
    D. Ward–Thompson

    Cardiff University, United Kingdom

    32 publications · 5.2K citations

    27

    h-index

  2. DA
    D. Arzoumanian

    Centre National de la Recherche Scientifique, France

    28 publications · 4K citations

    23

    h-index

  3. VK
    V. Könyves

    Astrophysique, Instrumentation et Modélisation, France

    23 publications · 3.5K citations

    22

    h-index

  4. JK
    J. Kainulainen

    Max Planck Institute for Astronomy, Germany

    22 publications · 1.3K citations

    20

    h-index

  5. FM
    F. Motte

    Centre National de la Recherche Scientifique, France

    20 publications · 4.8K citations

    20

    h-index

1–5 of 8.7K

Venues

  1. The Astrophysical Journal

    ApJ · 546 publications · 49.9K citations

    97

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    336 publications · 22.9K citations

    74

    h-index

  3. Astronomy and Astrophysics

    223 publications · 17.7K citations

    66

    h-index

  4. Physical Review Letters

    PRL · 48 publications · 3.5K citations

    35

    h-index

  5. The Astronomical Journal

    AJ · 50 publications · 3.4K citations

    32

    h-index

1–5