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