X-ray Reflection

X-Ray Reflection is a theoretical framework in high-energy astrophysics that describes the process by which X-rays emitted from an accreting compact object in a binary system are scattered and reprocessed by surrounding accretion disk material, producing characteristic spectral features such as the Compton hump and iron Kα emission line.

1.9K

Publications

111.6K

Citations

4.9K

Authors

1.2K

Institutions

Publications per year

2017–2026

259

Authors

4.9K

  1. AC
    A. C. Fabian

    University of Cambridge, United Kingdom

    91 publications · 10.2K citations

    49

    h-index

  2. JA
    Javier A. García

    California Institute of Technology, United States

    46 publications · 3.8K citations

    28

    h-index

  3. TD
    Thomas Dauser

    Friedrich-Alexander-Universität Erlangen-Nürnberg, Germany

    29 publications · 3.4K citations

    26

    h-index

  4. JM
    J. M. Mïller

    University of Michigan, United States

    33 publications · 2.5K citations

    25

    h-index

  5. GM
    G. Matt

    Roma Tre University, Italy

    28 publications · 2K citations

    24

    h-index

1–5 of 4.9K

Venues

  1. The Astrophysical Journal

    ApJ · 154 publications · 12K citations

    61

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    190 publications · 15.5K citations

    61

    h-index

  3. Physical review. B, Condensed matter

    PRB · 54 publications · 4.2K citations

    34

    h-index

  4. Astronomy and Astrophysics

    60 publications · 2.9K citations

    33

    h-index

  5. Spectrochimica Acta Part B Atomic Spectroscopy

    90 publications · 2.6K citations

    30

    h-index

1–5