Euphonious
发表于 2025-3-27 00:42:45
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反复无常
发表于 2025-3-27 04:44:57
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conjunctiva
发表于 2025-3-27 07:00:31
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vascular
发表于 2025-3-27 10:59:07
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无表情
发表于 2025-3-27 16:25:09
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拱墙
发表于 2025-3-27 20:30:24
Humans, Transhumans and Humanoids,on is discussed which may achieve higher maximum energy and maintain for a short period of time high cosmic ray luminosities. Accelerated cosmic rays will interact on the material of the supernova shell and give rise to high energy neutrino and γ-ray signals.
indignant
发表于 2025-3-28 02:01:06
https://doi.org/10.1007/978-3-319-95702-9. Emission from the southern extension of the remnant generally has a steeper radio spectrum than the north, with α up to ≈ 0.55. These results are discussed in relation to available theories for the radio emission from supernova remnants, and to the radio structure of the remnant.
领带
发表于 2025-3-28 05:27:33
Ralph O. Schill,Steffen Hengherr-3, Her X-1, Vela X-1 and Cen X-3 and of the radio pulsar sources PSR 0531 +21 and PSR 0833-45, the Crab and the Vela pulsars, are described in more detail. Possible VHE and UHE gamma ray source catalogs are examined. The current state and future requirements of VHE and UHE gamma ray astronomy are briefly discussed.
道学气
发表于 2025-3-28 08:13:34
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Peristalsis
发表于 2025-3-28 13:11:29
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