2007A&A...475..243D

The quest for hot dust in the central region of debris disks requires high resolution and high dynamic range imaging. Near-infrared interferometry is a powerful means to directly detect faint emission from hot grains. We probed the first 3AU around τ Ceti and ε Eridani with the CHARA array (Mt Wilson, USA) in order to gauge the 2µm excess flux emanating from possible hot dust grains in the debris disks and to also resolve the stellar photospheres. High precision visibility amplitude measurements were performed with the FLUOR single mode fiber instrument and telescope pairs on baselines ranging from 22 to 241m of projected length. The short baseline observations allow us to disentangle the contribution of an extended structure from the photospheric emission, while the long baselines constrain the stellar diameter. We have detected a resolved emission around τ Cet, corresponding to a spatially integrated, fractional excess flux of 0.98±0.21x10^–2 with respect to the photospheric flux in the K'-band. Around ε Eri, our measurements can exclude a fractional excess of greater than 0.6x10^–2 (3σ). We interpret the photometric excess around τ Cet as a possible signature of hot grains in the inner debris disk and demonstrate that a faint, physical or background, companion can be safely excluded. In addition, we measured both stellar angular diameters with an unprecedented accuracy: Θ_LD(τCet)=2.015±0.011mas and Θ_LD(εEri)=2.126±0.014mas.