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.
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2017–2026
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Nova‐induced Mass Transfer Variations
U. Kolb, S. Rappaport, K. Schenker et al. · The Astrophysical Journal · 2001 · 27 citations · Full text
Natural Sciences, Astronomy, Physics +13
L. Schmidtobreick, Michael M. Shara, C. Tappert et al. · Monthly Notices of the Royal Astronomical Society · 2015 · 20 citations · Full text
Natural Sciences, Astronomy, Physics +10
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Ecole Nationale d'Ingénieurs de Monastir
Monastir, Tunisia
1 h-index
1 publications
11 citations
Max Planck Institute for Astronomy
Heidelberg, Germany
1 h-index
1 publications
20 citations

University of Leicester
Leicester, United Kingdom
1 h-index
1 publications
27 citations

The Open University
Milton Keynes, United Kingdom
1 h-index
1 publications
27 citations
Instituto Español de Oceanografía
Madrid, Spain
1 h-index
2 publications
120 citations
Stanford University
Stanford, United States
1 h-index
5 publications
125 citations
Leiden University
Leiden, The Netherlands
1 h-index
1 publications
23 citations
École Nationale d'Ingénieurs de Gabès
Gabès, Tunisia
1 h-index
1 publications
11 citations
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2 publications · 43 citations
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ApJ · 1 publications · 27 citations
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1 publications · 60 citations
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1 publications · 25 citations
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1 publications · 11 citations
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