X-ray Coronae

X-Ray Coronae is a high-energy astrophysical phenomenon characterized by a diffuse, hot plasma surrounding compact objects or active galactic nuclei, distinguished by its emission in the X-ray spectrum due to thermal bremsstrahlung and inverse Compton scattering processes.

536

Publications

35K

Citations

1.3K

Authors

477

Institutions

Publications per year

2017–2026

118

Authors

1.3K

  1. AC
    A. C. Fabian

    University of Cambridge, United Kingdom

    28 publications · 2K citations

    23

    h-index

  2. JH
    J. H. M. M. Schmitt

    Universität Hamburg, Germany

    18 publications · 827 citations

    16

    h-index

  3. JA
    Javier A. García

    California Institute of Technology, United States

    16 publications · 822 citations

    15

    h-index

  4. MG
    M. Güdel

    University of Vienna, Austria

    15 publications · 1.5K citations

    14

    h-index

  5. GM
    G. Matt

    Roma Tre University, Italy

    13 publications · 579 citations

    13

    h-index

1–5 of 1.3K

Venues

  1. The Astrophysical Journal

    ApJ · 204 publications · 17.4K citations

    67

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    123 publications · 7.7K citations

    48

    h-index

  3. Astronomy and Astrophysics

    60 publications · 2.2K citations

    30

    h-index

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

    Repository · 15 publications · 880 citations

    14

    h-index

  5. Solar Physics

    11 publications · 725 citations

    11

    h-index

1–5