Figure 1 from New Evidence for a Substellar Luminosity Problem: Dynamical Mass for the Brown Dwarf Binary Gl 417BC

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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 1.

Contour plots of our Keck LGS AO images from which we derive astrometry and flux ratios (Table 1). Contours are in logarithmic intervals from unity to 7% of the peak flux in each band. The image cutouts are all the same size and have the same native pixel scale, and we have rotated them such that north is up for display purposes.

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