Paper:	Mass Loss from Massive Zero–Metallicity Stars
Volume:	353, Stellar Evolution at Low Metallicity: Mass Loss, Explosions, Cosmology
Page:	133
Authors:	Krticka, J.; Kubat, J.
Abstract:	We show that the radiative force is not able to drive a stellar wind from non-rotating hot massive zero-metallicity stars. This means that stellar winds from stationary massive hot first generation stars are unlikely. We study the possibility of expulsion of chemically homogeneous winds and the role of minor isotopes.

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