Bulge Stellar Orbits

Bulge Stellar Orbits is a theoretical construct in astrophysics that describes the characteristic trajectories of stars within the galactic bulge, distinguished by their predominantly radial and anisotropic motions influenced by the bulge’s non-axisymmetric gravitational potential.

41

Publications

2.2K

Citations

117

Authors

86

Institutions

Publications per year

2017–2026

11

Authors

117

  1. ÁP
    Ángeles Pérez-Villegas

    Universidade de São Paulo, Brazil

    3 publications · 174 citations

    3

    h-index

  2. OG
    Ortwin Gerhard

    Max Planck Institute for Extraterrestrial Physics, Germany

    3 publications · 232 citations

    3

    h-index

  3. RM
    R. Michael Rich

    University of California, Los Angeles, United States

    3 publications · 188 citations

    3

    h-index

  4. JS
    Juntai Shen

    Shanghai Astronomical Observatory, China

    3 publications · 94 citations

    3

    h-index

  5. EM
    E. Moreno

    Universidad Nacional Autónoma de México, Mexico

    3 publications · 140 citations

    3

    h-index

1–5 of 117

Venues

  1. 11

    h-index

  2. The Astrophysical Journal

    ApJ · 9 publications · 583 citations

    9

    h-index

  3. The Astrophysical Journal Letters

    5 publications · 258 citations

    5

    h-index

  4. The Astronomical Journal

    AJ · 4 publications · 217 citations

    4

    h-index

  5. Nature

    2 publications · 304 citations

    2

    h-index

1–5