Doppler Tomography

Doppler Tomography is a spectroscopic imaging technique that reconstructs the two-dimensional velocity structure of a rotating accretion disk or stellar surface by analyzing the time-resolved Doppler shifts of spectral lines across multiple orbital or rotational phases.

204

Publications

9.8K

Citations

769

Authors

348

Institutions

Publications per year

2017–2026

34

Authors

769

  1. ZC
    Zhongping Chen

    University of California, Irvine, United States

    17 publications · 1.8K citations

    15

    h-index

  2. JS
    J. Stuart Nelson

    University of California, Irvine, United States

    14 publications · 1.6K citations

    13

    h-index

  3. DS
    D. Steeghs

    University of Warwick, United Kingdom

    14 publications · 476 citations

    13

    h-index

  4. TR
    T. R. Marsh

    University of Warwick, United Kingdom

    14 publications · 1K citations

    13

    h-index

  5. DR
    Douglas R. Gies

    Georgia State University, United States

    15 publications · 453 citations

    13

    h-index

1–5 of 769

Venues

  1. Monthly Notices of the Royal Astronomical Society

    46 publications · 2.1K citations

    26

    h-index

  2. The Astrophysical Journal

    ApJ · 36 publications · 1.4K citations

    22

    h-index

  3. Astronomy and Astrophysics

    13 publications · 432 citations

    13

    h-index

  4. The Astronomical Journal

    AJ · 12 publications · 463 citations

    12

    h-index

  5. Optics Letters

    8 publications · 1.5K citations

    8

    h-index

1–5