The difference in mass loss between O and Of stars

Statistics – Computation

Scientific paper

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O Stars, Stellar Atmospheres, Stellar Evolution, Stellar Mass Ejection, Spectrum Analysis, Stellar Models, Stellar Spectrophotometry, Stochastic Processes

Scientific paper

The large difference in mass loss between O and Of stars cannot be explained by the small difference in radiation pressure. It is shown that the difference can be explained by a new theory, based on stochastic accelerations in a stellar photosphere. In combination with evolution computations, this theory corroborates the view that Of stars are evolved O stars.

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