A dust-driven streaming instability amplifies magnetic fields downstream of supernova remnant shocks and can account for observed X-ray filaments without upstream amplification.
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New LOFAR radio data and X-ray modeling indicate the extended source is thermal ICM emission from a massive merging galaxy cluster, unrelated to 1LHAASO J0343+5254u.
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Dust-driven streaming instability and magnetic field amplification downstream of supernova remnant shocks
A dust-driven streaming instability amplifies magnetic fields downstream of supernova remnant shocks and can account for observed X-ray filaments without upstream amplification.
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Multi-wavelength insights into the pulsar wind nebula candidate near 1LHAASO J0343+5254u: an obscured merging galaxy cluster?
New LOFAR radio data and X-ray modeling indicate the extended source is thermal ICM emission from a massive merging galaxy cluster, unrelated to 1LHAASO J0343+5254u.