Looking for Mister Goodstar (A preliminary analysis of stars with S IV, V and VI wind lines)

Abstract

The winds of stars with very specific temperatures and luminosities are ideal for determining the magnitude and nature of mass loss in OB stars. I identify these stars and analyze their wind lines. The results are discussed within the context of recent findings which appear to indicate that the mass-loss rates of OB stars may as much as an order of magnitude less than commonly accepted values.

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