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Mass loss from Wolf-Rayet stars
Authors:Mahendra Singh  U S Chaubey
Institution:(1) Uttar Pradesh State Observatory, Manora Peak, Naini Tal, India
Abstract:The observed times of minimum light derived from the photometry of the Wolf-Rayet eclipsing binary stars CQ Cep and V444 Cyg are used to estimate the mass-loss rate of the Wolf-Rayet components in several modes of mass-loss and mass-exchange.
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