X-ray detection of M~1.3 merger shock in A2142, reproduced by off-axis merger simulations, with radio arcs interpreted as shock-induced vortex rings and ultra-long tails explained by post-shock electron re-acceleration and plasma stretching.
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2 Pith papers cite this work. Polarity classification is still indexing.
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Overview of synergies between SKA radio observations and gamma-ray facilities for studying transient, variable, and steady GeV-TeV sources.
citing papers explorer
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A merger shock traced by radio arcs and ultra-long radio tails in galaxy cluster A2142
X-ray detection of M~1.3 merger shock in A2142, reproduced by off-axis merger simulations, with radio arcs interpreted as shock-induced vortex rings and ultra-long tails explained by post-shock electron re-acceleration and plasma stretching.
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SKAO and Gamma-Ray Synergies
Overview of synergies between SKA radio observations and gamma-ray facilities for studying transient, variable, and steady GeV-TeV sources.