Dynamical Parallax

Dynamical Parallax is a method in astrophysics that determines the distance to a binary star system by combining observational measurements of its orbital parameters and apparent brightness with Keplerian dynamics and mass-luminosity relations to infer parallax indirectly.

57

Publications

2.9K

Citations

169

Authors

96

Institutions

Publications per year

2017–2026

7

Authors

169

  1. JÁ
    J. Á. Docobo

    Universidade de Santiago de Compostela, Spain

    3 publications · 52 citations

    3

    h-index

  2. ND
    Norair D. Melikian

    Special Astrophysical Observatory, Russia

    3 publications · 52 citations

    3

    h-index

  3. VS
    V. S. Tamazian

    Universidade de Santiago de Compostela, Spain

    3 publications · 52 citations

    3

    h-index

  4. JS
    James S. Tittle

    The Ohio State University, United States

    2 publications · 91 citations

    2

    h-index

  5. MS
    M. Scardia

    Brera Astronomical Observatory, Italy

    2 publications · 39 citations

    2

    h-index

1–5 of 169

Venues

  1. The Astrophysical Journal

    ApJ · 16 publications · 1.5K citations

    14

    h-index

  2. The Astronomical Journal

    AJ · 9 publications · 245 citations

    9

    h-index

  3. 6

    h-index

  4. Publications of the Astronomical Society of the Pacific

    PASP · 4 publications · 88 citations

    4

    h-index

  5. Astronomy and Astrophysics

    4 publications · 170 citations

    4

    h-index

1–5