articleAstronomy and AstrophysicsJan 1, 2026DIAMOND OA

The ALMA survey to Resolve exoKuiper belt Substructures (ARKS)

JMJ. MilliJOJ. OlofssonMBM. BonduelleRBRaphaël Bendahan-WestJPJ. P. Marshall

Centre National de la Recherche Scientifique · Université Grenoble Alpes · +32 more institutions

Indexed inarxivcrossrefdoaj

Abstract

Context . Debris discs are analogues to our own Kuiper belt around main-sequence stars and are therefore referred to as exoKuiper belts. They have been resolved at high angular resolution at wavelengths spanning the optical/near-infrared to the submillimetre-millimetre regime. Short wavelengths can probe the light scattered by such discs, which is dominated by micron-sized dust particles, while millimetre wavelengths can probe the thermal emission of millimetre-sized particles. Determining differences in the dust distribution between millimetre- and micron-sized dust is fundamental to revealing the dynamical processes affecting the dust in debris discs. Aims . We aim to compare the scattered light from the…

Citation impact

6
total citations
FWCI
72.06
Percentile
100%
References
125
Too recent for citation history.

Authors

36

Topics & keywords

Topics
Keywords
  • Planet
  • Wavelength
  • Exoplanet
  • Stars
  • Cosmic dust
  • Angular resolution (graph drawing)
  • Circumstellar dust
  • Thermal
No related works found for this paper.

Funding