A cocoon of freshly accelerated cosmic rays detected by Fermi in the Cygnus superbubble
The origin of Galactic cosmic rays is a century-long puzzle. Indirect evidence points to their acceleration by supernova shockwaves, but we know little of their escape from the shock and their evolution through the turbulent medium surrounding massive stars. Gamma rays can probe their spreading thro...
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| Vydané v: | Science (American Association for the Advancement of Science) Ročník 334; číslo 6059; s. 1103 |
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| Hlavní autori: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
| Médium: | Journal Article |
| Jazyk: | English |
| Vydavateľské údaje: |
United States
25.11.2011
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| ISSN: | 1095-9203, 1095-9203 |
| On-line prístup: | Zistit podrobnosti o prístupe |
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