Convective Driving

Convective Driving is a physical mechanism in stellar astrophysics whereby pulsations in certain types of variable stars are sustained by the modulation of convective energy transport in response to oscillation-induced changes in the stellar envelope's thermodynamic state.

33

Publications

1.7K

Citations

101

Authors

70

Institutions

Publications per year

2017–2026

7

Authors

101

  1. MD
    M.‐A. Dupret

    University of Liège, Belgium

    3 publications · 342 citations

    3

    h-index

  2. AG
    A. Grigahcène

    Instituto de Astrofísica de Andalucía, Spain

    3 publications · 492 citations

    3

    h-index

  3. RS
    R. Scuflaire

    University of Liège, Belgium

    2 publications · 472 citations

    2

    h-index

  4. RG
    R. Garrido

    Instituto de Astrofísica de Andalucía, Spain

    2 publications · 472 citations

    2

    h-index

  5. MG
    M. Gabriel

    University of Liège, Belgium

    2 publications · 472 citations

    2

    h-index

1–5 of 101

Venues

  1. The Astrophysical Journal

    ApJ · 6 publications · 305 citations

    6

    h-index

  2. Astronomy and Astrophysics

    6 publications · 579 citations

    6

    h-index

  3. 2

    h-index

  4. Journal of Climate

    1 publications · 27 citations

    1

    h-index

  5. 1

    h-index

1–5