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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https://doi.org/10.1007/978-94-009-8500-1Accretion; Galaxy; star; stars; stellar

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Effects of Mass Loss on Stellar Evolution978-94-009-8500-1Series ISSN 0067-0057 Series E-ISSN 2214-7985

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https://doi.org/10.1007/978-1-4842-3159-3erved in the ultraviolet with IUE. From an analysis of the UV spectra we determine a terminal velocity of 3560 ± 100 km s. and a mass loss rate of (4.2 .) 10. M. yr.. A comparison is made with the stars of similar spectral type.

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植物茂盛

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Organizing and Managing Queries,In addition to certain manifestation of a stellar wind during steady states of WR-stars that we have heard here about I have two notes on their extremal stages of evolution which may be also connected to such a hydrodynamical event.

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A survey of Clustering AlgorithmsAG Car is a variable supergiant surrounded by a small ring nebula. Its ultraviolet and optical spectrum, and UV to IR energy distribution are similar to those of P Cyg with v. = -290 km s.. Also the strength of the 2200 A band is the same and suggests E(B-V) = 0.55 both stars. The possible variability of the infrared flux is discussed.