Mass Transfer Variability

Mass Transfer Variability is a stellar variability mechanism, distinguished from other such mechanisms by its dependence on the intermittent or asymmetric exchange of mass between binary star components, which modulates luminosity, spectral features, and orbital dynamics over time.

6

Publications

166

Citations

28

Authors

20

Institutions

Publications per year

2017–2026

0

Authors

28

  1. UK
    U. Kolb

    The Open University, United Kingdom

    1 publications · 27 citations

    1

    h-index

  2. AB
    A. Bayo

    University of Valparaíso, Chile

    1 publications · 20 citations

    1

    h-index

  3. SB
    Steve B. Howell

    Ames Research Center, United States

    1 publications · 27 citations

    1

    h-index

  4. PS
    Pablo Sangrà

    Universidad de Las Palmas de Gran Canaria, Spain

    1 publications · 60 citations

    1

    h-index

  5. SG
    Stephen G. Monismith

    Stanford University, United States

    1 publications · 25 citations

    1

    h-index

1–5 of 28

Venues

  1. 2

    h-index

  2. The Astrophysical Journal

    ApJ · 1 publications · 27 citations

    1

    h-index

  3. 1

    h-index

  4. Journal of Geophysical Research Oceans

    1 publications · 25 citations

    1

    h-index

  5. Drying Technology

    1 publications · 11 citations

    1

    h-index

1–5