  We have found a photoevaporated disk in the Orion Nebula that includes a wide
binary. HST/ACS observations of the proplyd 124-132 show two point-like sources
separated by 0".15, or about 60 AU at the distance of Orion. The two sources
have nearly identical I and z magnitudes. We analyze the brightest component,
Source N, comparing the observed magnitudes with those predicted using a 1 Myr
Baraffe/NEXTGEN isochrone with different accretion luminosities and
extinctions. We find that a low mass (\simeq 0.04 M_\odot) brown dwarf ~1 Myr
old with mass accretion rate \log\dot{M}\simeq -10.3, typical for objects of
this mass, and about 2 magnitudes of visual extinction provides the best fit to
the data. This is the first observation of a circumbinary disk undergoing
photoevaporation and, if confirmed by spectroscopic observations, the first
direct detection of a wide substellar pair still accreting and enshrouded in
its circumbinary disk.
