Warm-hot Intergalactic Medium

Warm-Hot Intergalactic Medium is a diffuse, ionized plasma phase of the intergalactic medium, distinguished by its temperature range of $10^5$ to $10^7$ K and its role in hosting a significant fraction of the baryonic matter in the low-redshift universe, primarily detectable through soft X-ray and ultraviolet absorption lines.

219

Publications

13.7K

Citations

480

Authors

283

Institutions

Publications per year

2017–2026

54

Variants

Whim

Authors

480

  1. TF
    Taotao Fang

    Xiamen University, China

    13 publications · 913 citations

    13

    h-index

  2. KM
    Kazuhisa Mitsuda

    Institute of Space and Astronautical Science, Japan

    11 publications · 291 citations

    11

    h-index

  3. JS
    Joop Schaye

    Leiden University, Netherlands

    11 publications · 709 citations

    10

    h-index

  4. SM
    Smita Mathur

    The Ohio State University, United States

    10 publications · 1.4K citations

    10

    h-index

  5. NY
    Noriko Y. Yamasaki

    Institute of Space and Astronautical Science, Japan

    10 publications · 236 citations

    10

    h-index

1–5 of 480

Venues

  1. The Astrophysical Journal

    ApJ · 67 publications · 5.5K citations

    39

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    47 publications · 2.7K citations

    31

    h-index

  3. Astronomy and Astrophysics

    20 publications · 1K citations

    18

    h-index

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

    Repository · 9 publications · 592 citations

    9

    h-index

  5. The Astrophysical Journal Letters

    9 publications · 476 citations

    9

    h-index

1–5