The first event-horizon-scale image of the M87 black hole shows a 42 microarcsecond diameter ring with a central brightness depression, consistent with the shadow of a Kerr black hole.
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2 Pith papers cite this work. Polarity classification is still indexing.
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LHAASO TeV sources associate with SNRs at 0.19, PWNe at 0.20, and microquasars at 0.027, with PWNe showing ~60% gamma-ray bright fraction and molecular clouds enhancing emission.
citing papers explorer
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First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole
The first event-horizon-scale image of the M87 black hole shows a 42 microarcsecond diameter ring with a central brightness depression, consistent with the shadow of a Kerr black hole.
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A Comparative Study of TeV Gamma-Ray Sources with Various Objects
LHAASO TeV sources associate with SNRs at 0.19, PWNe at 0.20, and microquasars at 0.027, with PWNe showing ~60% gamma-ray bright fraction and molecular clouds enhancing emission.