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Determining the Masses and Evolution of CVs through Ellipsoidal Variations
Published online by Cambridge University Press: 22 February 2018
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We use simultaneous multi-wavelength BVRI-JHK photometric observations of cataclysmic variables (CVs) to determine the inclination angles of the systems, together with phase-resolved spectroscopy to calculate the K2 and vsini. We then calculate the masses of the system components. We are using these data to construct mass-radius diagrams of the secondaries in an effort to resolve some of the debate over their evolutionary history.
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- Copyright © Instituto de astronomia/revista mexicana de astronomίa y astrofίsica 2004
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