Resolving the cold debris disc around a planet-hosting star . PACS photometric imaging observations

@article{Liseau2010ResolvingTC,
  title={Resolving the cold debris disc around a planet-hosting star . PACS photometric imaging observations},
  author={Ren{\'e} Liseau and Carlos Eiroa and Davide Fedele and J. C. Augereau and G̈oran Olofsson and B. Gonzalez and J. Maldonado and Benjam{\'i}n Montesinos and Alejandro Mora and Olivier Absil and David Ardila and David Tejerina Barrado and Amelia Bayo and Charles Arnold Beichman and Geoffrey C. Bryden and William C. Danchi and Carlos del Burgo and Steve Ertel and C. W. M. Fridlund and Ana M. Heras and Alexander V. Krivov and Ralf Launhardt and J{\'e}r{\'e}my Lebreton and Torsten Lohne and Jonathan Marshall and G Meeus and Sebastian Andreas Muller and Goeran L. Pilbratt and Aki Roberge and Jens Rodmann and Enrique Solano and Karl R. Stapelfeldt and Ph.Th'ebault and Glenn J. White and Sebastian G. Wolf},
  journal={Astronomy and Astrophysics},
  year={2010}
}
  • René Liseau, Carlos Eiroa, +32 authors Sebastian G. Wolf
  • Published 2010
  • Physics
  • Astronomy and Astrophysics
  • Context. About two dozen exo-solar debris systems have been spatially resolved. These debris discs commonly display a variety of structural features such as clumps, rings, belts, excentric distributions and spiral patterns. In most cases, these features are believed to be formed, shaped and maintained by the dynamical influence of planets orbiting the host stars. In very few cases has the presence of the dynamically important planet(s) been inferred from direct observation. Aims. The solar-type… CONTINUE READING

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