闲聊 发表于 2025-3-26 22:04:25
https://doi.org/10.1007/3-540-56432-2CCD; LOPES; Population; Sternentwicklung; Supernova; astrophysics; chemical abundances; chemische HäufigkeiNOT 发表于 2025-3-27 01:13:35
http://reply.papertrans.cn/67/6649/664850/664850_32.pngRange-Of-Motion 发表于 2025-3-27 07:30:05
http://reply.papertrans.cn/67/6649/664850/664850_33.pngBUOY 发表于 2025-3-27 12:33:55
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http://reply.papertrans.cn/67/6649/664850/664850_35.pngCougar 发表于 2025-3-27 19:07:03
http://reply.papertrans.cn/67/6649/664850/664850_36.pngphase-2-enzyme 发表于 2025-3-28 00:43:22
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http://reply.papertrans.cn/67/6649/664850/664850_38.pngLignans 发表于 2025-3-28 07:48:36
Deep infrared images of the Small Magellanic Cloud and comparison with the distribution of ultraviostrong correlation between the far infrared and the ultraviolet emission but the dispersion in this correlation is unrelated to infrared colors. Comparing with the results for the nearby spiral M33 at different radial distances, it is suggested that the population of dust grains in the Small Magellaexcursion 发表于 2025-3-28 10:41:52
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