赏心悦目 发表于 2025-3-25 05:53:26

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NUDGE 发表于 2025-3-25 10:55:29

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entice 发表于 2025-3-25 13:49:43

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银版照相 发表于 2025-3-25 16:14:18

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落叶剂 发表于 2025-3-25 20:07:31

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Arbitrary 发表于 2025-3-26 02:40:19

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无力更进 发表于 2025-3-26 08:16:36

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中止 发表于 2025-3-26 09:46:51

https://doi.org/10.1007/978-3-642-18636-3its small, but measurable diffusivity. Collectively, results point to the GB(4.4, 20.0, 1.0, 1.0) parameterization as being a better candidate in capturing the typical gamut of liquid crystalline phases.

消息灵通 发表于 2025-3-26 16:16:43

Harmful Algal Blooms in a Changing Oceanon pressure may not be the physical mechanism that determines how massive stars can become. Here we find using frequency-dependent radiation transfer calculations, coupled to a frequency-dependent dust model, that stellar masses in excess of 100 . may well form by runaway accretion in a collapsing,

Cocker 发表于 2025-3-26 20:43:58

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查看完整版本: Titlebook: Experimental and Theoretical Advances in Fluid Dynamics; Jaime Klapp,Anne Cros,Mario Alberto Rodriguez Meza Book 2012 The Editor(s) (if ap