The supernova remnant SN 1006 as a Galactic particle accelerator
It is known that cosmic rays could be accelerated by shock waves in supernova (SN) remnants. Here, the authors show that SN 1006 remnant is an efficient source of cosmic rays, providing observational support for the quasi-parallel acceleration mechanism.
| Glavni autori: | , , , , , , , , |
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| Format: | Članak |
| Jezik: | English |
| Izdano: |
Nature Portfolio
2022-08-01
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| Serija: | Nature Communications |
| Online pristup: | https://doi.org/10.1038/s41467-022-32781-4 |
| Sažetak: | It is known that cosmic rays could be accelerated by shock waves in supernova (SN) remnants. Here, the authors show that SN 1006 remnant is an efficient source of cosmic rays, providing observational support for the quasi-parallel acceleration mechanism. |
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| ISSN: | 2041-1723 |