Titlebook: Mass Loss from Red Giants; Proceedings of a Con Mark Morris,Ben Zuckerman Conference proceedings 1985 D. Reidel Publishing Company, Dordrec

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Jacques M. Beckers analyses ranging from sample extraction to higher-throughput metabolite annotation. With the integrated UHPLC-QTOF-MS/MS-SPE-NMR method, we have purified and confidently identified more than 100 previously known as well as unknown triterpene and flavonoid glycosides while noting that most of the id

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A. L. Betz,D. M. Goldhaberironment. Such a theory was developed by Shimshoni and Stern (SS) [.]. The SS theory takes into account the dephasing effect due to stochastic field fluctuations. Combining this theory with measurements of dephasing times for MM could lead to a revision in tunnel splitting calculations. But, as far

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Kenneth H. Hinkleironment. Such a theory was developed by Shimshoni and Stern (SS) [.]. The SS theory takes into account the dephasing effect due to stochastic field fluctuations. Combining this theory with measurements of dephasing times for MM could lead to a revision in tunnel splitting calculations. But, as far

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R. Sahai,Alwyn Wootten,R. E. S. Cleggwritten for the natural scientist who is well versed in mathematics and physics. Assumptions are made and terms are used that would not be appro- priate for a medical or biochemical text. The goal of this introduc- tion, therefore, is to discuss the principles of the NMR technique in terms that are meaningful978-3-540-13442-8978-3-642-69741-8

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On the Significance of Mass Loss from Bright Red Giants,erflow, most intermediate-mass stars in close binaries become white dwarfs; perhaps 10 percent of all white dwarf pairs formed in this way are close enough that gravitational wave radiation will lead to merging of the white dwarfs; 10 percent of the merging dwarfs become type I supernovae.