Resolved Spectroscopy of a Brown Dwarf Binary at the T Dwarf/Y Dwarf Transition

We report resolved near-infrared imaging and spectroscopic observations of the T8.5 binary WISEP J045853.90+643452.6AB obtained with Keck/NIRC2, Keck/OSIRIS, and the Keck Laser Guide Star Adaptive Optics system. These data confirm common proper and radial motion for the two components, and we see the first indications of orbital motion (mostly radial) for this system. H-band spectroscopy identifies both components as very late type brown dwarfs with strong H_2O and CH_4 absorption. The spectrum of WISE J0458+6434B also exhibits a compelling signature of NH_3 absorption over 1.52-1.54 μm when compared to the T9 dwarf UGPS J072227.51–054031.2. Comparison to T8-Y0 spectral standards and H-band spectral indices indicate classifications of T8.5 and T9.5 for these two components, approaching the boundary between the T dwarf and Y dwarf spectral classes