A nine-epoch uGMRT campaign detects no star-planet interaction radio emission from GJ 486; if the signal is intrinsically faint, the stellar mass-loss rate is below about 0.3 solar and the Poynting-to-radio efficiency below about 10^-3.
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Searching for star-planet interactions in GJ 486 at radio wavelengths with the uGMRT
A nine-epoch uGMRT campaign detects no star-planet interaction radio emission from GJ 486; if the signal is intrinsically faint, the stellar mass-loss rate is below about 0.3 solar and the Poynting-to-radio efficiency below about 10^-3.