Spectral energy distribution simulations of a possible ring structure around the young, red brown dwarf G 196-3 B
The origin of the very red optical and infrared colours of intermediate-age (˜10-500 Myr) L-type dwarfs remains unknown. It has been suggested that low-gravity atmospheres containing large amounts of dust may account for the observed reddish nature. We explored an alternative scenario by simulating debris disc around G 196-3 B, which is an L3 young
Zakhozhay, O. V. et al.
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2017