Stellar Hydrostatic Equilibrium

Stellar Hydrostatic Equilibrium is a theoretical construct in astrophysics denoting the state in which the inward gravitational force at every point within a star is exactly balanced by the outward pressure gradient force, thereby maintaining the star's stable, spherical structure against collapse or expansion.

316

Publications

19.1K

Citations

723

Authors

365

Institutions

Publications per year

2017–2026

84

Authors

723

  1. JD
    José D. V. Arbañil

    Private University of the North, Peru

    7 publications · 316 citations

    7

    h-index

  2. JM
    Juan M. Z. Pretel

    Centro Brasileiro de Pesquisas Físicas, Brazil

    7 publications · 259 citations

    7

    h-index

  3. AB
    Ayan Banerjee

    University of KwaZulu-Natal, South Africa

    5 publications · 464 citations

    5

    h-index

  4. MM
    M. Malheiro

    Instituto Tecnológico de Aeronáutica, Brazil

    4 publications · 409 citations

    4

    h-index

  5. SK
    S. K. Maurya

    University of Nizwa, Oman

    4 publications · 415 citations

    4

    h-index

1–5 of 723

Venues

  1. The Astrophysical Journal

    ApJ · 94 publications · 5K citations

    42

    h-index

  2. Astronomy and Astrophysics

    28 publications · 2K citations

    24

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    42 publications · 1.6K citations

    22

    h-index

  4. The European Physical Journal C

    17 publications · 735 citations

    14

    h-index

  5. 12

    h-index

1–5