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Titlebook: Algols; Proceedings of the 1 Alan H. Batten Conference proceedings 1989 Springer Science+Business Media Dordrecht 1989 CCD.accretion disk.g

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期刊全称Algols
期刊简称Proceedings of the 1
影响因子2023Alan H. Batten
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图书封面Titlebook: Algols; Proceedings of the 1 Alan H. Batten Conference proceedings 1989 Springer Science+Business Media Dordrecht 1989 CCD.accretion disk.g
影响因子When leaving the Victoria airport the day before our Colloquium, I saw a van of the Dunsmuir Lodge marked with big letters which I read as "Alcohol Colloquium". I do often make such blunders because of the global, casual, and careless way in which I read various ads, and checked myself quickly to read it correctly as "Algol Colloquium". Millions of fellow citizens could easily make the same mistake, and no apology could be expected. Even I read and hear the word alcohol more frequently than Algol, although I must say that Algols have given me more pleasure and fewer headaches over the years; in that, however, I may be a singularity, and possibly a pitiful one at that. Being appointed Chairman of the Scientific Organizing Committee, I may be deemed to be a purer" Algolist" than other investigators, although my range of active interests is much broader; and the same is true about all the 28 invited speakers and all the other participants of the Colloquium. Our interest are strongly diversified, but there are several good reasons that brought us together at this Colloquium.
Pindex Conference proceedings 1989
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Elektronische Konstruktionskomponenten,atural to look at the rotation statistics of Algols to test this idea. The badly behaved light curves and spectroscopy of some Algols (eg. U Cep, RZ Sct) may be attributable to the double contact condition, and the ramifications of this possibility are discussed. If so, the rotation statistics of Al
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The H, Emitting Regions of the Accretion Disks in Algols,r - q diagram has the largest influence on its behavior. The . side of the accretion disk, where the gas stream impacts the inner disk, is usually brighter, and the . side is often times more extended. The disk extends out to at least 95%of the Roche surface of the primary and is highly flattened (≤
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Algol, Beta Lyrae, and W Serpentis: Some New Results for Three Well Studied Eclipsing Binaries,published ., and H-alpha index light curves of W Ser are presented and discussed. W Ser is a very complex binary system that undergoes complicated, large changes in its light curves. The physical properties of W Ser are only poorly known, but it probably contains one component at its Roche surface,
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