An interferometric study of the Fomalhaut inner debris disk: III. Detailed models of the exozodiacal disk and its origin

@article{Lebreton2013AnIS,
  title={An interferometric study of the Fomalhaut inner debris disk: III. Detailed models of the exozodiacal disk and its origin},
  author={J{\'e}r{\'e}my Lebreton and Rik van Lieshout and J. Ch. Augereau and Olivier Absil and Bertrand Mennesson and Mihkel Kama and Carsten Dominik and Amy Bonsor and Julien Vandeportal and Herv'e Beust and Denis Defr{\`e}re and Steve Ertel and Virginie Faramaz and Philip M. Hinz and Quentin Kral and Anne-Marie Lagrange and W. Liu and Ph. Th'ebault},
  journal={Astronomy and Astrophysics},
  year={2013},
  volume={555}
}
Context. Debris disks are thought to be extrasolar analogs to the solar system planetesimal belts. The star Fomalhaut harbors a cold debris belt at 140 AU comparable to the Edgeworth-Kuiper belt, as well as evidence of a warm dust component, unresolved by singledish telescopes, which is suspected of being a bright analog to the solar system’s zodiacal dust. Aims. Interferometric observations obtained with the VLTI/VINCI instrument and the Keck Interferometer Nuller have identified nearand mid… Expand
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TLDR
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