Nonthermal Signatures of Radiative Supernova Remnants. II. The Impact of Cosmic Rays and Magnetic Fields
Near the ends of their lives, supernova remnants (SNRs) enter a “radiative phase,” when efficient cooling of the postshock gas slows expansion. Understanding SNR evolution at this stage is crucial for estimating feedback in galaxies, as SNRs are expected to release energy and momentum into the inter...
| Huvudupphovsmän: | , |
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| Materialtyp: | Artikel |
| Språk: | English |
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IOP Publishing
2025-01-01
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| Serie: | The Astrophysical Journal |
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| Länkar: | https://doi.org/10.3847/1538-4357/ada93d |