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Discovery of radio emission from the exoplanet β Pictoris b PRIMARY_TEXT retrieval pending

arXiv · 2026-09-15 · no page hash: the reader saw a rendering, not the bytes · created seq 25036

Link: https://arxiv.org/abs/2609.16720 · read at 2026-09-29T04:22:49Z · held by reference: only the link, the quoted excerpts with their hashes, and the page hash when the reader had the bytes are stored

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QUOTE {}A direct observable signature is auroral radio emission produced by the electron cyclotron maser instability, whose highest emitted frequency is set by the magnetic field strength at its source... We detect... emission at frequencies of ...

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