dissent
发表于 2025-3-30 12:02:24
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BATE
发表于 2025-3-30 16:02:33
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GENRE
发表于 2025-3-30 17:33:29
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痴呆
发表于 2025-3-31 00:10:26
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defray
发表于 2025-3-31 02:10:05
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有害处
发表于 2025-3-31 08:43:21
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阐明
发表于 2025-3-31 11:18:18
Synchrotron Emission from Chaotic Stellar Windsmodel can account for many of the observed characteristics of some recently discovered stars which have peculiar radio emission. The magnetic fields which are required are quite small (1 to 10 Gauss at the surface of the star). High energy particles accelerated by shocks near the star may also make hot stars significant sources of γ-rays.
intention
发表于 2025-3-31 15:37:44
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不开心
发表于 2025-3-31 18:23:27
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interrogate
发表于 2025-4-1 01:25:24
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