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Titlebook: Currents in High-Energy Astrophysics; Maurice M. Shapiro,Rein Silberberg,John P. Wefel Book 1995 Springer Science+Business Media Dordrecht

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發(fā)表于 2025-3-21 19:04:57 | 只看該作者 |倒序瀏覽 |閱讀模式
書目名稱Currents in High-Energy Astrophysics
編輯Maurice M. Shapiro,Rein Silberberg,John P. Wefel
視頻videohttp://file.papertrans.cn/242/241513/241513.mp4
叢書名稱Nato Science Series C:
圖書封面Titlebook: Currents in High-Energy Astrophysics;  Maurice M. Shapiro,Rein Silberberg,John P. Wefel Book 1995 Springer Science+Business Media Dordrecht
出版日期Book 1995
關(guān)鍵詞Big Bang; Cosmology; EFE; Galaxy; Quasar; Star; Universe; astronomy; astrophysics
版次1
doihttps://doi.org/10.1007/978-94-011-0253-7
isbn_softcover978-94-010-4112-6
isbn_ebook978-94-011-0253-7Series ISSN 1389-2185
issn_series 1389-2185
copyrightSpringer Science+Business Media Dordrecht 1995
The information of publication is updating

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Verbeter de zorg met inzichten uit dataom observations accumulated over the last two decades, and then discusses some of the latest observations, focusing on recent interpretations of the data, and theoretical approaches that may help unravel the mysteries of gamma-ray bursts.
板凳
發(fā)表于 2025-3-22 02:12:11 | 只看該作者
Ga met elkaar om de tekentafel zittenting in the large halo. If this explanation of the detected flux is viable, the . result will be the first detection of a truly diffuse extragalactic Compton emission, underlining the significance of the escape of cosmic ray electrons from galaxies, and highlighting the interest in starburst galaxies for the study of this and related phenomena.
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“COЮЗ PYCCKИX PEBOЛЮЦИOHHЫX ГPYПп”(“COЮЗ”),), in the processes of cosmic ray acceleration by shock waves and in regions of magnetic field reconnection. Here we will consider general characteristics of cosmic ray nonlinear effects and its application to the dynamic processes in the galactic halo.
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發(fā)表于 2025-3-22 17:21:53 | 只看該作者
The Sky as viewed from the Compton Gamma Ray Observatory the reason for doing astronomy in the gamma ray energy range, the questions on which this discipline got started and why it took a long time before the present mature state as a member in the spectrum of multiwavelength astronomers was reached.
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