Spectrum and Location of Ongoing Extreme Particle Acceleration in Cassiopeia A
Young supernova remnants (SNRs) are believed to be the origin of energetic cosmic rays (CRs) below the “knee” of their spectrum at ∼3 PeV (10 ^15 eV). Nevertheless, the precise location, duration, and operation of CR acceleration in young SNRs are open questions. Here, we report on multiepoch X-ray...
| প্রধান লেখক: | , , , , , , , , , , |
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| বিন্যাস: | প্রবন্ধ |
| ভাষা: | English |
| প্রকাশিত: |
IOP Publishing
2025-01-01
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| মালা: | The Astrophysical Journal |
| বিষয়গুলি: | |
| অনলাইন ব্যবহার করুন: | https://doi.org/10.3847/1538-4357/ad98f1 |