CURD
发表于 2025-3-21 20:05:13
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MOTIF
发表于 2025-3-21 21:52:09
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overhaul
发表于 2025-3-22 03:13:40
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GLADE
发表于 2025-3-22 06:58:07
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CONE
发表于 2025-3-22 11:28:34
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挖掘
发表于 2025-3-22 16:45:38
1389-2185 ded as comingofage. Pul sars and accreting neutron stars have now been studied at every wavelength, from the initial radio observations, through optical, X-, and "{-ray, up to the very recent observations in the TeV region, while theorists have studied in some detail relevant physical processes bot
常到
发表于 2025-3-22 20:55:58
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POINT
发表于 2025-3-22 22:36:05
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束以马具
发表于 2025-3-23 02:54:12
Neutron Star Formation in Close Binary Systems. The light curves of SNe Ib/Ic (maximum brightness and decline rate) are used to infer the progenitors’ masses and the neutron star masses. (3) Thirdly the evolutionary origin of double neutron stars are discussed in relation to SNe Ib/Ic.
angiography
发表于 2025-3-23 07:53:23
An Introduction to Matter at Subnuclear Densitiess, the surface tension of neutron-rich and hot nuclei, the reduction of the Coulomb energy as a consequence of the close packing of nuclei, and the possibility of non-spherical nuclei. For the most part, the discussion of nuclear properties is based on generalizations of the liquid-drop model, but r