喃喃而言 发表于 2025-3-26 21:32:07
Georg Toepfern, allerdings auch für astronomische Verhältnisse recht langlebigen „Zwischenzustände“ behandeln wir in diesem Kapitel. Verschiedene Formen stehen dabei im Vordergrund. Wir diskutieren kompakte Objekte wie Weiße Zwerge und Neutronensterne, aber auch Quasare und Schwarze Löcher. Aber letztlich werdenHARP 发表于 2025-3-27 02:16:02
http://reply.papertrans.cn/43/4275/427482/427482_32.pngchronicle 发表于 2025-3-27 06:00:37
http://reply.papertrans.cn/43/4275/427482/427482_33.png最有利 发表于 2025-3-27 09:26:46
http://reply.papertrans.cn/43/4275/427482/427482_34.pngFLORA 发表于 2025-3-27 14:17:08
http://reply.papertrans.cn/43/4275/427482/427482_35.pngDefault 发表于 2025-3-27 19:02:41
Georg Toepfernd spectra. Theoretical development in model stellar atmospheres, in the theory of line broadening, and more data on parallaxes are badly needed. Nevertheless we now approach a period in which interpretation of white-dwarf spectra in terms of composition will become profitable.Hypopnea 发表于 2025-3-27 23:12:07
http://reply.papertrans.cn/43/4275/427482/427482_37.png过时 发表于 2025-3-28 02:54:51
Georg Toepfert was also a significant milestone for Bayesian astrostatistics, as this research area was chosen as a (non-exclusive) focus for the session..As an early (and elder!) proponent of Bayesian methods in astronomy, I have been asked to provide a “perspective piece” on the history and status of Bayesianoverture 发表于 2025-3-28 06:42:56
http://reply.papertrans.cn/43/4275/427482/427482_39.png炼油厂 发表于 2025-3-28 11:32:34
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