Stellar Pulsation Effects

Stellar Pulsation Effects is a physical phenomenon in stellar atmospheres characterized by periodic expansions and contractions of a star’s outer layers driven by internal pressure and opacity instabilities, leading to observable variations in luminosity, temperature, and radial velocity.

101

Publications

5.2K

Citations

301

Authors

186

Institutions

Publications per year

2017–2026

10

Authors

301

  1. SH
    S. Höfner

    Uppsala University, Sweden

    5 publications · 272 citations

    5

    h-index

  2. PJ
    P. J. Diamond

    SKA Observatory, United Kingdom

    5 publications · 264 citations

    5

    h-index

  3. GH
    G. H. Bowen

    Iowa State University, United States

    4 publications · 229 citations

    4

    h-index

  4. LA
    L. A. Balona

    South African Radio Astronomy Observatory, South Africa

    3 publications · 104 citations

    3

    h-index

  5. MB
    M. Breger

    University of Vienna, Austria

    3 publications · 429 citations

    3

    h-index

1–5 of 301

Venues

  1. Astronomy and Astrophysics

    27 publications · 1.8K citations

    22

    h-index

  2. 15

    h-index

  3. The Astrophysical Journal

    ApJ · 13 publications · 397 citations

    12

    h-index

  4. Springer Link (Chiba Institute of Technology)

    Repository · 5 publications · 342 citations

    5

    h-index

  5. Communications in Asteroseismology

    CoAst · 3 publications · 56 citations

    3

    h-index

1–5