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1. Quantitative spectroscopy of stellar atmospheres and clumped hot star winds - new methods and first results for deriving mass-loss rates.


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2. Constraining general massive-star physics by exploring the unique properties of magnetic O-stars: Rotation, macroturbulence, and sub-surface convection


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3. Clumping in the inner winds of hot, massive stars from hydrodynamical line-driven instability simulations


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4. Clumping in the inner winds of hot, massive stars from hydrodynamical line-driven instability simulations


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5. Clumping in the inner winds of hot, massive stars from hydrodynamical line-driven instability simulations


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6. A proper description of clumping in hot star winds: the key to obtaining reliable mass-loss rates?


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7. OB-stars as extreme condition test beds


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8. The Physical Basis of the Lx-Lbol Empirical Law for O-star X-rays


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9. The nature and consequences of clumping in hot, massive star winds


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10. A generalized porosity formalism for isotropic and anisotropic effective opacity and its effects on X-ray line attenuation in clumped O star winds


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