Titlebook: Diffuse Matter from Star Forming Regions to Active Galaxies; A Volume Honouring J T.W. HARTQUIST,J.M. PITTARD,S.A.E.G. FALLE Book 2007 Spri

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Approximations Based on De Pril TransformsThe formation and evolution of massive (> 10M.) stars plays a key role in the final fate of their parental molecular clouds, and in the appearance and evolution of their host galaxies.

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The Time-Series Estimation ProblemMost stars will experience episodes of substantial mass loss at some point in their lives. For very massive stars, mass loss dominates their evolution, although the mass loss rates are not known exactly, particularly once the star has left the main sequence.

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