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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書(shū)目名稱Currents in High-Energy Astrophysics影響因子(影響力)

書(shū)目名稱Currents in High-Energy Astrophysics影響因子(影響力)學(xué)科排名

書(shū)目名稱Currents in High-Energy Astrophysics網(wǎng)絡(luò)公開(kāi)度

書(shū)目名稱Currents in High-Energy Astrophysics網(wǎng)絡(luò)公開(kāi)度學(xué)科排名

書(shū)目名稱Currents in High-Energy Astrophysics被引頻次

書(shū)目名稱Currents in High-Energy Astrophysics被引頻次學(xué)科排名

書(shū)目名稱Currents in High-Energy Astrophysics年度引用

書(shū)目名稱Currents in High-Energy Astrophysics年度引用學(xué)科排名

書(shū)目名稱Currents in High-Energy Astrophysics讀者反饋

書(shū)目名稱Currents in High-Energy Astrophysics讀者反饋學(xué)科排名

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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.

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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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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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