The nature of mid-infrared excesses from hot dust around Sun-like stars

@article{Smith2008TheNO,
  title={The nature of mid-infrared excesses from hot dust around Sun-like stars},
  author={R. Smith and M. Wyatt and W. Dent},
  journal={Astronomy and Astrophysics},
  year={2008},
  volume={485},
  pages={897-915}
}
Aims. Studies of the debris disk phenomenon have shown that most systems are analogous to the Edgeworth-Kuiper Belt (EKB). However a rare subset of sun-like stars possess dust which lies, in contrast, in the terrestrial planet region. In this study we aim to determine how many sources with apparent mid-infrared excess are truly hosts of warm dust, and investigate where the dust in these systems must lie. Methods. We observed using ground-based mid-infrared imaging with TIMMI2, VISIR and… Expand
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