Fast 21-micron flaring and a flat radio-to-mid-infrared spectrum show that the mid-infrared excess in the quiescent black hole binary V404 Cygni comes from a persistent relativistic jet.
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The Mid-infrared Emitting Jet in the Black Hole V404 Cygni in Quiescence
Fast 21-micron flaring and a flat radio-to-mid-infrared spectrum show that the mid-infrared excess in the quiescent black hole binary V404 Cygni comes from a persistent relativistic jet.