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New Evidence for a Substellar Luminosity Problem: Dynamical Mass for the Brown Dwarf Binary Gl 417BC

  • Authors: Trent J. Dupuy, Michael C. Liu, and Michael J. Ireland

Dupuy, Liu, & Ireland 2014 The Astrophysical Journal 790 133.

  • Provider: AAS Journals

Caption: Figure 2.

Left: relative astrometry for Gl 417BC along with our best-fit orbit. Error bars for the data are smaller than the plotting symbols. The short dotted line indicates the time of periastron passage, the long dashed line shows the line of nodes, and small empty circles show predicted future locations. Right: measurements of the projected separation and P.A. of Gl 417BC. The best-fit orbit is shown as a solid line. The bottom panels show the observed minus computed (O − C) measurements with observational error bars.

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