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.
主要な著者: | Roberta Giuffrida, Marco Miceli, Damiano Caprioli, Anne Decourchelle, Jacco Vink, Salvatore Orlando, Fabrizio Bocchino, Emanuele Greco, Giovanni Peres |
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フォーマット: | 論文 |
言語: | English |
出版事項: |
Nature Portfolio
2022-08-01
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シリーズ: | Nature Communications |
オンライン・アクセス: | https://doi.org/10.1038/s41467-022-32781-4 |
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