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The dynamical mass of a classical Cepheid variable star in an eclipsing binary systems
(2010)
Stellar pulsation theory provides a means of determining the masses of pulsating classical Cepheid supergiants—it is the pulsation that causes their luminosity to vary. Such pulsational masses are found to be smaller than ...
Eclipsing post-common envelope binaries from the catalina surveys
(OXFORD UNIV PRESS, 2013)