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Optical Spectroscopy of CH Cygni in 1985/86
Published online by Cambridge University Press: 12 April 2016
Abstract
Some arguments for the explanation of the spectroscopic and photometric behavior of CH Cyg in terms of an eclipsing binary with P=5700 days, consisting of M6 III star and an accreting white dwarf, are presented. Physical and geometrical parameters of the system have been estimated and discussed.
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- VII. Related Objects
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- Copyright © Reidel 1987
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