Galactic X-ray Background

The Galactic X-Ray Background is a diffuse astronomical phenomenon constituting a component of the X-ray background radiation that originates from within the Milky Way galaxy, primarily due to thermal emission from hot interstellar plasma and unresolved populations of X-ray-emitting stars and compact objects, thereby distinguishing it from extragalactic X-ray background sources.

327

Publications

21.3K

Citations

1.1K

Authors

316

Institutions

Publications per year

2017–2026

23

Variants

Galactic X-ray Background Radiation

Authors

1.1K

  1. RS
    R. Sunyaev

    Space Research Institute, Russia

    16 publications · 880 citations

    15

    h-index

  2. EC
    E. Churazov

    Max Planck Institute for Astrophysics, Germany

    14 publications · 905 citations

    14

    h-index

  3. HB
    H. Bradt

    Massachusetts Institute of Technology, United States

    11 publications · 436 citations

    11

    h-index

  4. EA
    E. A. Boldt

    Goddard Space Flight Center, United States

    11 publications · 601 citations

    11

    h-index

  5. QD
    Q. Daniel Wang

    University of Massachusetts Amherst, United States

    10 publications · 381 citations

    10

    h-index

1–5 of 1.1K

Venues

  1. The Astrophysical Journal

    ApJ · 140 publications · 10K citations

    48

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    40 publications · 2.8K citations

    28

    h-index

  3. Nature

    29 publications · 2.1K citations

    21

    h-index

  4. Astronomy and Astrophysics

    26 publications · 1.9K citations

    21

    h-index

  5. 10

    h-index

1–5