entail 发表于 2025-3-30 09:42:20
On the Internal Structure of Main-Sequence Starse variations in relative positions of the eclipses and the comparison with different theoretical models, we could deduce that the discrepancy, previously reported by several authors between theory and observations, is no longer supported. Moreover, a strong correlation has been found between the evo态度暖昧 发表于 2025-3-30 13:59:24
A Study of the Orbital Periods of 22 Eclipsing Binariesetecting additional components in them. Systematic study of the period changes in binary stars was started by Plavec (Plavec et al 1960) more than twenty years ago. Work on the same lines for 20 detached systems was reported by Herczeg (1980) at the I.A.U. Symposium No. 88 held in Toronto two years染色体 发表于 2025-3-30 19:50:03
http://reply.papertrans.cn/19/1863/186289/186289_53.pngLoathe 发表于 2025-3-31 00:47:33
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http://reply.papertrans.cn/19/1863/186289/186289_55.pngMacronutrients 发表于 2025-3-31 08:35:02
http://reply.papertrans.cn/19/1863/186289/186289_56.pngBlood-Vessels 发表于 2025-3-31 12:25:30
http://reply.papertrans.cn/19/1863/186289/186289_57.png手铐 发表于 2025-3-31 14:49:46
Evolution of Stars in the Post-Main Sequence Stagethe main sequence and to march towards the region of the red supergiants the methods known at that time failed to produce models. For less massive stars the exhaustion of hydrogen could be followed up more easily and, in 1955, the great paper by Hoyle and Schwarzschild came out, which showed how thePriapism 发表于 2025-3-31 19:36:22
On the Distribution of Young Spectroscopic Binary Stars over the Major Semiaxes of their Orbitsticlopidine 发表于 2025-3-31 22:54:19
Binary and Multiple Stars as Tracers of Stellar EvolutionProceedings of the 6