Interstellar Medium Structure

Interstellar Medium Structure is a physical construct that characterizes the spatial and phase distribution of gas and dust within the Galactic Disk, differentiating itself from other components of Milky Way Structure by detailing the morphology, density, temperature, and ionization states of the material filling the space between stars.

504

Publications

35.5K

Citations

1.5K

Authors

504

Institutions

Publications per year

2017–2026

89

Authors

1.5K

  1. DJ
    D. J. McComas

    Southwest Research Institute, United States

    21 publications · 1.6K citations

    18

    h-index

  2. NA
    N. A. Schwadron

    University of New Hampshire, United States

    19 publications · 1.1K citations

    15

    h-index

  3. JL
    Jeffrey L. Linsky

    Joint Institute for Laboratory Astrophysics, United States

    15 publications · 1.7K citations

    15

    h-index

  4. RL
    R. Lallement

    Centre National de la Recherche Scientifique, France

    16 publications · 817 citations

    14

    h-index

  5. SR
    Seth Redfield

    Wesleyan University, United States

    13 publications · 1.4K citations

    13

    h-index

1–5 of 1.5K

Venues

  1. The Astrophysical Journal

    ApJ · 178 publications · 15.2K citations

    62

    h-index

  2. Astronomy and Astrophysics

    46 publications · 3.4K citations

    31

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    40 publications · 1.3K citations

    23

    h-index

  4. The Astrophysical Journal Letters

    29 publications · 1.5K citations

    23

    h-index

  5. The Astronomical Journal

    AJ · 15 publications · 761 citations

    13

    h-index

1–5