infarct 发表于 2025-3-23 09:48:43
http://reply.papertrans.cn/16/1529/152815/152815_11.png烧烤 发表于 2025-3-23 15:07:40
The Relation of Algols and W Serpentis Stars,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 AlDENT 发表于 2025-3-23 21:12:02
The Relation Between RS CVn and Algol,s these changes. Specifically, the interval from one increase (or decrease) to the next can be equated with the star’s magnetic cycle. Cycle lengths for 31 stars, derived in this way, range between 7 years and 109 years, with a median of 50 years.控制 发表于 2025-3-24 01:18:26
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. Eve退潮 发表于 2025-3-24 05:32:44
Ludger Deters Prof. Dr.-Ing.,Dirk Bartelfrom the binary system. The mass flow is not conservative. During the phase of dynamic mass flow, the companion star becomes immersed in optically-thick plasma and the physical properties of that star elude close scrutiny.Hay-Fever 发表于 2025-3-24 08:09:09
http://reply.papertrans.cn/16/1529/152815/152815_16.pngEsalate 发表于 2025-3-24 14:17:59
Grundlagen der Strömungsmaschinenroblem of the initial parameters of Algol systems. For the latter, a search is made for conservative case B systems. UZ Cyg seems to be a good candidate for such evolution. Finally, some remarks are given on the initial values of the low mass Algol S Cancri.Irritate 发表于 2025-3-24 15:47:00
http://reply.papertrans.cn/16/1529/152815/152815_18.png懒惰民族 发表于 2025-3-24 22:41:59
http://reply.papertrans.cn/16/1529/152815/152815_19.pngWordlist 发表于 2025-3-25 00:30:06
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