案发地点
发表于 2025-3-23 12:55:35
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声明
发表于 2025-3-23 16:41:27
,Summary and Future Prospects,here planetesimals form are not smooth profile as assumed in the classical standard theory but quite structured. Especially, dust rings and gaps have been frequently observed, which might be the key to explain dust growth toward planetesimals in protoplanetary disks. In this thesis, we investigate d
HUSH
发表于 2025-3-23 20:04:36
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insecticide
发表于 2025-3-24 01:25:25
Ryosuke TominagaHighlights new instability triggered by dust-gas friction and turbulent viscosity.Presents a new instability driven by dust coagulation in protoplanetary disks.Offers a planetesimal formation scenario
提升
发表于 2025-3-24 02:23:50
Springer Theseshttp://image.papertrans.cn/e/image/283450.jpg
COM
发表于 2025-3-24 07:37:36
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Nmda-Receptor
发表于 2025-3-24 12:35:35
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terazosin
发表于 2025-3-24 18:45:07
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Preamble
发表于 2025-3-24 21:17:33
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男学院
发表于 2025-3-25 01:05:05
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