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Post Info TOPIC: WISEP J061135.13-041024.0


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WISEP J061135.13-041024.0
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Title: WISEP J061135.13-041024.0AB: A J-Band Flux Reversal Binary at the L/T Transition.
Author: Christopher R. Gelino, R. L. Smart, Federico Marocco, J. Davy Kirkpatrick, Michael C. Cushing, Gregory Mace, Rene A. Mendez, C. G. Tinney, Hugh R. A. Jones

We present Keck II laser guide star adaptive optics observations of the brown dwarf WISEP J061135.13-041024.0 showing it is a binary with a component separation of 0.4". This system is one of the six known resolved binaries in which the magnitude differences between the components show a reversal in sign between the Y/J band and the H/K bands. Deconvolution of the composite spectrum results in a best fit binary solution with L9 and T1.5 components. We also present a preliminary parallax placing the system at a distance of 21.2+/-1.3 pc. Using the distance and resolved magnitudes we are able to place WISEP J061135.13-041024.0AB on a color-absolute magnitude diagram, showing that this system contributes to the well-known "J-band bump" and the components' properties appear similar to other late-type L and early-type T dwarfs. Fitting our data to a set of cloudy atmosphere models suggests the system has an age >1 Gyr with WISEP J061135.13-041024.0A having an effective temperature (Teff) of 1275-1325 K and mass of 64-65 M_Jup, and WISEP J061135.13-041024.0B having Teff = 1075-1115 K and mass 40-65 M_Jup.

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