University of Hertfordshire

From the same journal

By the same authors

Documents

  • Christopher R. Gelino
  • R. L. Smart
  • Federico Marocco
  • Davy Kirkpatrick
  • Michael C. Cushing
  • Gregory Mace
  • Rene A. Mendez
  • C. G. Tinney
  • Hugh Jones
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Original languageEnglish
Number of pages10
JournalAstronomical Journal
Volume148
Issue6
DOIs
Publication statusPublished - 28 May 2014

Abstract

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 J061135.13−041024.0 AB 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 WISE 0611−0410 A having an effective temperature (Teff) of 1275–1325 K and mass of 64–65 MJup, and WISE 0611−0410 B having Teff = 1075–1115 K and mass 40–65 MJup.

Notes

Christopher R. Gelino, et al, 'WISEP J061135.13−041024.0 AB: A J-BAND FLUX REVERSAL BINARY AT THE L/T TRANSITION', The Astronomical Journal, vol. 148 (6), July 2014, doi: http://dx.doi.org/10.1088/0004-6256/148/1/6.

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