Titlebook: Effects of Mass Loss on Stellar Evolution; IAU Colloquium no. 5 C. Chiosi,R. Stalio Book 1981 D. Reidel Publishing Company, Dordrecht, Holl

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Book 1981related to the problem of mass loss from stars - would have spurred thorough discussions on the many aspects and implications of this topic. We hope this goal has been achieved. Furthermore, the most recent observational and theoreti- cal developments on the problem of mass loss from early ty- pe st

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Summary, Conclusions, and Future Work,the WR mass loss may also be important for Of stars (Lamers 1980). A determination of the properties of the WR stellar winds will provide diagnostics which might aid in identifying the mass loss mechanism, and P-Cygni profiles form one important data source for this purpose. With the advent of IUE m

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An Introduction to Data Mining,± 100 km s.. Our preliminary evaluation of the associated mass loss rate gives 10. M. yr.. Other planetary nebulae nuclei are studied with low resolution IUE spectra and indications are found of mass loss rates consistent with the above value.