极深 发表于 2025-3-23 10:41:05
Bertil Haack,Ulrike Tippe,Michael Stobernack,Tilo Wendler and the graphs are compiled in the present subvolume c. For the user‘s convenience, special indexes of (a) gross molecular formulas, (b) chemical substance names, and (c) CAS Registry Numbers of all substances considered are added at the end of this subvolume.978-3-540-47990-1Series ISSN 1615-1844 Series E-ISSN 1616-9522公式 发表于 2025-3-23 15:05:52
Bertil Haack,Ulrike Tippe,Michael Stobernack,Tilo Wendler and the graphs are compiled in the present subvolume c. For the user‘s convenience, special indexes of (a) gross molecular formulas, (b) chemical substance names, and (c) CAS Registry Numbers of all substances considered are added at the end of this subvolume.978-3-540-47990-1Series ISSN 1615-1844 Series E-ISSN 1616-9522谷类 发表于 2025-3-23 21:20:15
http://reply.papertrans.cn/63/6273/627249/627249_13.pnginitiate 发表于 2025-3-23 23:06:47
http://reply.papertrans.cn/63/6273/627249/627249_14.pngosteoclasts 发表于 2025-3-24 03:57:52
http://reply.papertrans.cn/63/6273/627249/627249_15.png听写 发表于 2025-3-24 09:35:42
Bertil Haack,Ulrike Tippe,Michael Stobernack,Tilo Wendler the role of the contributing source(s) of .-process elements. Our main findings are that in addition to neutron star mergers, a second, early acting site is necessary. We assume “magnetorotationally driven supernovae” as this additional and earlier r-process site and conclude that our simulations w雪上轻舟飞过 发表于 2025-3-24 14:16:02
Bertil Haack,Ulrike Tippe,Michael Stobernack,Tilo Wendler the role of the contributing source(s) of .-process elements. Our main findings are that in addition to neutron star mergers, a second, early acting site is necessary. We assume “magnetorotationally driven supernovae” as this additional and earlier r-process site and conclude that our simulations w孤独无助 发表于 2025-3-24 15:24:07
http://reply.papertrans.cn/63/6273/627249/627249_18.png新字 发表于 2025-3-24 22:05:34
http://reply.papertrans.cn/63/6273/627249/627249_19.pngDOSE 发表于 2025-3-25 00:05:24
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