cumulative
发表于 2025-3-25 04:24:25
radio emission is indicative of high energy, nonthermal processes: acceleration of electrons to some 10‘s of keV or, in some circumstances, several MeV or more. These electrons then emit radio waves by the incoherent processes of gyroresonance and gyrosynchrotron radiation, and the coherent process
Abrade
发表于 2025-3-25 07:39:19
Patrick Millot radio emission is indicative of high energy, nonthermal processes: acceleration of electrons to some 10‘s of keV or, in some circumstances, several MeV or more. These electrons then emit radio waves by the incoherent processes of gyroresonance and gyrosynchrotron radiation, and the coherent process
意见一致
发表于 2025-3-25 14:57:24
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Gesture
发表于 2025-3-25 18:41:45
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bile648
发表于 2025-3-25 20:44:47
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轻浮思想
发表于 2025-3-26 00:49:42
Boris Kryzhanovsky,Vladimir Kryzhanovsky,Andrey Mikaelianncluding the Orion, Taurus-Auriga, ρ Ophiuchi and Chamaeleon clouds obtained with the Einstein X-ray Observatory have revealed more than 150 X-ray luminous PMS stars to date. Some are classical strong emission line T Tauri stars while others are late-type PMS stars with weak or absent lines. The sof
infarct
发表于 2025-3-26 06:37:48
Nicolas Jouandeauncluding the Orion, Taurus-Auriga, ρ Ophiuchi and Chamaeleon clouds obtained with the Einstein X-ray Observatory have revealed more than 150 X-ray luminous PMS stars to date. Some are classical strong emission line T Tauri stars while others are late-type PMS stars with weak or absent lines. The sof
大范围流行
发表于 2025-3-26 10:40:01
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discord
发表于 2025-3-26 13:44:49
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平
发表于 2025-3-26 19:38:43
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