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Very recently, a second companion on wider orbit has been discovered aroundGQ Lup. This is a low-mass accreting star partially obscured by a disk seen athigh inclination. If detected, this disk may be compared to the known diskaround the primary. We detected this disk on archive HST and WISE data. Theextended spectral energy distribution provided by these data confirms thepresence of accretion from Halpha emission and UV excess, and shows an IRexcess attributable to a warm disk. In addition, we resolved the disk on theHST images. This is found to be roughly aligned with the disk of the primary.Both of them are roughly aligned with the Lupus I dust filament containing GQLup.

The disk of 2MASS 15491331-3539118 = GQ Lup C as seen by HST and WISE