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Paper: Winds and the underlying physical parameters of hot stars - an observational approach
Volume: 7, Properties of Hot Luminous Stars: Boulder-Munich Workshop
Page: 294
Authors: Corcoran, M. F.; Heap, S. R.
Abstract: The predicted values of wind terminal velocity calculated using the formalism of Kudritzki et al. (1989) are compared with observed values for 4 OB binaries with well determined component masses, radii, and temperatures. The aim is to derive the value of the force multiplier parameter alpha appropriate to the winds from these stars.
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