The only inflated brown dwarf in an eclipsing white dwarf–brown dwarf binary: WD1032+011B
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DOI: 10.1093/mnras/stae2121
Abstract: Due to their short orbital periods and relatively high flux ratios, irradiated brown dwarfs in binaries with white dwarfs offer better opportunities to study irradiated atmospheres than hot Jupiters, which have lower planet-to-star flux ratios.… read more here.
Keywords: wd1032 011b; dwarf; white dwarf; dwarf brown ... See more keywords