Stellar Stability

Stellar Stability is a theoretical construct in astrophysics that characterizes the capacity of a star to maintain hydrostatic equilibrium against gravitational collapse or explosive expansion through the balance of internal pressure and gravitational forces.

490

Publications

29.4K

Citations

749

Authors

386

Institutions

Publications per year

2017–2026

144

Authors

749

  1. MS
    M. Sharif

    University of the Punjab, Pakistan

    19 publications · 592 citations

    15

    h-index

  2. SK
    S. K. Maurya

    University of Nizwa, Oman

    10 publications · 467 citations

    10

    h-index

  3. MF
    M. Farasat Shamir

    National University of Computer and Emerging Sciences, Pakistan

    8 publications · 232 citations

    8

    h-index

  4. AM
    Adnan Malik

    University of Management and Technology, Pakistan

    8 publications · 318 citations

    8

    h-index

  5. NS
    N. Sanchis-Gual

    Universitat de València, Spain

    7 publications · 406 citations

    7

    h-index

1–5 of 749

Venues

  1. The Astrophysical Journal

    ApJ · 101 publications · 9.1K citations

    39

    h-index

  2. 31

    h-index

  3. The European Physical Journal C

    25 publications · 1K citations

    19

    h-index

  4. 18

    h-index

  5. Physical review. D/Physical review. D.

    PRD · 20 publications · 809 citations

    16

    h-index

1–5