Time-resolved observations of brown dwarfs' rotational modulations provide powerful insights into the properties of condensate clouds in ultra-cool atmospheres. Multi-wavelength light curves reveal cloud vertical structures, condensate particle sizes, and cloud morphology, which directly constrain condensate cloud and atmospheric circulation models. We report results from Hubble Space Telescope/Wide Field Camera 3 near-infrared G141 taken in six consecutive orbits observations of HN Peg B, an L/T transition brown dwarf companion to a G0V type star. The best-fit sine wave to the 1.1 − 1.7µm broadband light curve has the amplitude of 1.206 ± 0.025% and period of 15.4 ± 0.5 hr. The modulation amplitude has no detectable wavelength dependence except in the 1.4 µm water absorption band, indicating that the characteristic condensate particle sizes are large (> 1µm). We detect significantly (4.4σ) lower modulation amplitude in the 1.4µm water absorption band, and find that HN Peg B's spectral modulation resembles those of early T type brown dwarfs. We also describe a new empirical interpolation method to remove spectral contamination from the bright host star. This method may be applied in other high-contrast time-resolved observations with WFC3.
|Original language||English (US)|
|State||Published - Jan 29 2018|
- Brown dwarfs
- Methods: observational
- Stars: atmospheres
ASJC Scopus subject areas