stars: individual: 99 Herculis, HD 165908, HIP 88745, GJ704AB

Introduction {#s:intro}
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The *Herschel* Key Program DEBRIS (Dust Emission via a Bias free Reconnaissance in the Infrared/Submillimeter) has observed a large sample of nearby stars to discover and characterise extrasolar analogues to the Solar System’s asteroid and Kuiper belts, collectively known as “debris disks.” The 3.5m *Herschel* mirror diameter provides 6-7” resolution at 70-100$\mu$m , and as a consequence our survey has resolved many disks around stars in the Solar neighbourhood for the first time .[^2]

Here we present resolved images of the 99 Herculis circumbinary disk. This system is particularly interesting because unlike most debris disk+binary systems, the binary orbit is well characterised. The combination of a known orbit and resolved disk means we can compare their (different) inclinations and consider circumbinary particle dynamics and formation scenarios.

This system is a first step toward building on the binary debris disk study of @2007ApJ...658.1289T. Their *Spitzer* study found that debris disks are as common in binary systems as in single systems, but tend not to have separations in the 3-30AU range. However, only some of their systems had detections at multiple wavelengths to constrain the disk location and none were 