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Methane emission from a cool brown dwarf - Nature

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Methane emission from a cool brown dwarf - Nature

Beyond our Solar System, aurorae have been inferred from radio observations of isolated brown dwarfs1,2. Within our Solar System, giant planets have auroral emission with signatures across the electromagnetic spectrum including infrared emission of H3+ and methane. Isolated brown dwarfs with auroral signatures in the radio have been searched for corresponding infrared features, but only null detections have been reported3.

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Methane emission from a cool brown dwarf - Nature

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Methane emission from a cool brown dwarf - Nature

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