Variability of the Lowest Mass Objects in the AB Doradus Moving Group
arXiv:1710.07194 · doi:10.1093/mnras/stx2752
Abstract
We present the detection of [m] photometric variability in two young, L/T transition brown dwarfs, WISE J004701.06+680352.1 (W0047) and 2MASS J2244316+204343 (2M2244) using the \textit{Spitzer Space Telescope}. We find a period of hr and a peak-to-peak amplitude of for W0047, and a period of hr and amplitude of for 2M2244. This period is significantly longer than that measured previously during a shorter observation. {We additionally detect significant -band variability in 2M2244 using the Wide-Field Camera on UKIRT. } We determine the radial and rotational velocities of both objects using Keck NIRSPEC data. We find a radial velocity of km s for 2M2244, and confirm it as a bona fide member of the AB Doradus moving group. We find rotational velocities of km sand km s for W0047 and 2M2244, respectively. With inclination angles of and , W0047 and 2M2244 are viewed roughly equator-on. Their remarkably similar colours, spectra and inclinations are consistent with the possibility that viewing angle may influence atmospheric appearance. We additionally present \textit{Spitzer} monitoring of the young, T5.5 object SDSS111010+011613 (SDSS1110) where we detect no variability. For periods hr, we place an upper limit of on the peak-to-peak variability amplitude of SDSS1110.
14 pages, Accepted for publication in MNRAS
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