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Titlebook: Cosmic Rays in Star-Forming Environments; Proceedings of the S Diego F. Torres,Olaf Reimer Conference proceedings 2013 Springer-Verlag Berl

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樓主: Taft
31#
發(fā)表于 2025-3-26 21:32:31 | 只看該作者
32#
發(fā)表于 2025-3-27 03:44:09 | 只看該作者
Conference proceedings 2013e a comprehensive review of the state of the field from the observational to the theoretical perspectives. In the meeting, the prospects for possible observations with planned instruments across the multi-wavelength spectrum were analyzed and also how they impact on our understanding of these systems..
33#
發(fā)表于 2025-3-27 08:41:06 | 只看該作者
34#
發(fā)表于 2025-3-27 11:02:17 | 只看該作者
35#
發(fā)表于 2025-3-27 16:20:44 | 只看該作者
1570-6591 2nd Workshop on Cosmic-ray Induced Phenomenology in Stellar Environments, held April 16-19, 2012. The aim of this Workshop was to address the current knowledge and challenges of high-energy emission from stellar environments at all scales and provide a comprehensive review of the state of the field
36#
發(fā)表于 2025-3-27 20:46:38 | 只看該作者
37#
發(fā)表于 2025-3-28 00:29:30 | 只看該作者
38#
發(fā)表于 2025-3-28 05:54:51 | 只看該作者
Web Information Systems and Technologiesory of diffusive shock acceleration has to be completed with an additional ingredient, which we propose to be the enhanced velocity of the magnetic irregularities particles scatter against, to reconcile the theory of efficient particle acceleration with recent observations of gamma-ray bright supernova remnants.
39#
發(fā)表于 2025-3-28 07:48:11 | 只看該作者
40#
發(fā)表于 2025-3-28 12:16:54 | 只看該作者
Space as the Next Theater of War,dentify CO, CO., SiO, S and O. as the main species that contribute to the gas extinction in these regions. The implementation of this method seeks to complete other models that use steady state estimations of the chemical composition of the disk.
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