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...
Saved in:
| Published in: | Science (American Association for the Advancement of Science) Vol. 334; no. 6059; p. 1103 |
|---|---|
| Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
| Format: | Journal Article |
| Language: | English |
| Published: |
United States
25.11.2011
|
| ISSN: | 1095-9203, 1095-9203 |
| Online Access: | Get more information |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Be the first to leave a comment!