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- W2111331999 abstract "I report on the X-ray detection of Gl 569Bab. During a 25 ks Chandra observation, the binary brown dwarf is for the first time spatially separated in X-rays from the flare star primary Gl 569A. Companionship to Gl 569A constrains the age of the brown dwarf pair to ~300-800 Myr. The observation presented here is only the second X-ray detection of an evolved brown dwarf. About half of the observing time is dominated by a large flare on Gl 569Bab; the remainder is characterized by weak and nonvariable emission just above the detection limit. This emission—if not related to the afterglow of the flare—represents the first detection of a quiescent corona on a brown dwarf, representing an important piece in the puzzle of dynamos in the substellar regime." @default.
- W2111331999 created "2016-06-24" @default.
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- W2111331999 date "2004-10-06" @default.
- W2111331999 modified "2023-10-16" @default.
- W2111331999 title "Quiescent X-Ray Emission from an Evolved Brown Dwarf?" @default.
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- W2111331999 doi "https://doi.org/10.1086/426121" @default.
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