A candidate brown dwarf appears to have a 1700 au long dust trail, possibly formed by external photoevaporation or by Bondi-Hoyle accretion.
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A possible trail of dust from a young, highly-extincted brown dwarf in the outskirts of the Trapezium Cluster
A candidate brown dwarf appears to have a 1700 au long dust trail, possibly formed by external photoevaporation or by Bondi-Hoyle accretion.