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- W2000269306 abstract "Masses are derived for the components of 10 short period cataclysmic variable stars. With one exception, the masses of the white dwarf primaries lie in the range 1.2 ± 0.2 M⊙ , and are thus approximately three times heavier than isolated white dwarf stars." @default.
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- W2000269306 date "1973-06-01" @default.
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- W2000269306 title "On the Masses of Cataclysmic Variable Stars" @default.
- W2000269306 doi "https://doi.org/10.1093/mnras/162.3.189" @default.
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