Stellar Proper Motion

Stellar Proper Motion is the apparent angular displacement of a star across the celestial sphere over time, as observed from the Solar System barycenter, distinguished from radial motion by its transverse component relative to the line of sight.

1K

Publications

67.2K

Citations

2.5K

Authors

735

Institutions

Publications per year

2017–2026

185

Authors

2.5K

  1. AG
    Andrew Gould

    The Ohio State University, United States

    15 publications · 772 citations

    14

    h-index

  2. JA
    Jay Anderson

    Space Telescope Science Institute, United States

    12 publications · 552 citations

    12

    h-index

  3. RP
    Roeland P. van der Marel

    Space Telescope Science Institute, United States

    12 publications · 1.1K citations

    12

    h-index

  4. MJ
    M. J. Reid

    Center for Astrophysics Harvard & Smithsonian, United States

    11 publications · 1.9K citations

    11

    h-index

  5. SR
    Steven R. Majewski

    University of Virginia, United States

    12 publications · 628 citations

    11

    h-index

1–5 of 2.5K

Venues

  1. The Astrophysical Journal

    ApJ · 285 publications · 25K citations

    79

    h-index

  2. The Astronomical Journal

    AJ · 146 publications · 8.7K citations

    51

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    142 publications · 9.4K citations

    48

    h-index

  4. Astronomy and Astrophysics

    128 publications · 7K citations

    47

    h-index

  5. The Astrophysical Journal Letters

    28 publications · 1.7K citations

    24

    h-index

1–5