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• W2265164019 abstract "The average white dwarf (WD) masses in cataclysmic variables (CVs) have been measured to significantly exceed those of single WDs, which is the opposite of what is theoretically expected. We present the results of binary population synthesis models taking into account consequential angular momentum loss (CAML) that is assumed to increase with decreasing WD mass. This approach can not only solve the WD mass problem, but also brings in agreement theoretical predictions and observations of the orbital period distribution and the space density of CVs. We speculate that frictional angular momentum loss following nova eruptions might cause such CAML and could thus be the missing ingredient of CV evolution." @default.
• W2265164019 created "2016-06-24" @default.
• W2265164019 creator A5001263708 @default.
• W2265164019 creator A5052396663 @default.
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• W2265164019 date "2015-10-20" @default.
• W2265164019 modified "2023-10-04" @default.
• W2265164019 title "Three in one go: consequential angular momentum loss can solve major problems of CV evolution" @default.
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• W2265164019 doi "https://doi.org/10.1093/mnrasl/slv144" @default.
• W2265164019 hasPublicationYear "2015" @default.
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