Warm Ionized Medium

Warm Ionized Medium is a phase of the diffuse interstellar medium characterized by its high ionization fraction and thermal temperature range of approximately 8,000 to 10,000 K, sustained primarily by photoionization from hot stars in the surrounding interstellar radiation field.

242

Publications

17.4K

Citations

609

Authors

346

Institutions

Publications per year

2017–2026

43

Variants

Wim

Authors

609

  1. LM
    L. M. Haffner

    University of Wisconsin–Madison, United States

    11 publications · 1.4K citations

    11

    h-index

  2. RJ
    R. J. Reynolds

    University of Wisconsin–Madison, United States

    9 publications · 387 citations

    9

    h-index

  3. BD
    Blair D. Savage

    University of Wisconsin–Madison, United States

    8 publications · 360 citations

    8

    h-index

  4. RJ
    R. J. Reynolds

    University of Wisconsin–Madison, United States

    8 publications · 1.4K citations

    8

    h-index

  5. JC
    J. Christopher Howk

    University of Notre Dame, United States

    6 publications · 490 citations

    6

    h-index

1–5 of 609

Venues

  1. The Astrophysical Journal

    ApJ · 98 publications · 7.7K citations

    47

    h-index

  2. Astronomy and Astrophysics

    24 publications · 1.5K citations

    19

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    26 publications · 1.5K citations

    18

    h-index

  4. The Astronomical Journal

    AJ · 8 publications · 407 citations

    8

    h-index

  5. 4

    h-index

1–5