H I Shells

H I Shells is a galactic-scale interstellar structure composed predominantly of neutral atomic hydrogen (H I), distinguished by its shell-like morphology resulting from supernova-driven expansion and stellar feedback processes within H I regions.

191

Publications

9.3K

Citations

479

Authors

271

Institutions

Publications per year

2017–2026

18

Authors

479

  1. CH
    Carl Heiles

    University of California, Berkeley, United States

    8 publications · 999 citations

    8

    h-index

  2. BK
    Bon‐Chul Koo

    Seoul National University, South Korea

    6 publications · 272 citations

    6

    h-index

  3. JI
    J. Irwin

    Queen's University, Canada

    5 publications · 193 citations

    5

    h-index

  4. JM
    J. M. van der Hulst

    University of Groningen, Netherlands

    5 publications · 412 citations

    5

    h-index

  5. LS
    L. Staveley‐Smith

    The University of Western Australia, Australia

    5 publications · 853 citations

    5

    h-index

1–5 of 479

Venues

  1. The Astrophysical Journal

    ApJ · 53 publications · 3.5K citations

    34

    h-index

  2. The Astronomical Journal

    AJ · 35 publications · 1.9K citations

    22

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    26 publications · 1.4K citations

    19

    h-index

  4. Astronomy and Astrophysics

    24 publications · 656 citations

    15

    h-index

  5. CERN Document Server (European Organization for Nuclear Research)

    Repository · 6 publications · 133 citations

    6

    h-index

1–5