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The ALMA survey to Resolve exoKuiper belt Substructures (ARKS)

Context. The outer regions of planetary systems host dusty debris discs analogous to the Kuiper belt (exoKuiper belts), which provide crucial constraints on planet formation and evolution processes. ALMA dust observations have revealed a great diversity in terms of radii, widths, and scale heights....

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Autori principali: Marino S., Matrà L., Hughes A. M., Ehrhardt J., Kennedy G. M., del Burgo C., Brennan A., Han Y., Jankovic M. R., Lovell J. B., Mac Manamon S., Milli J., Weber P., Zawadzki B., Bendahan-West R., Fehr A., Mansell E., Olofsson J., Pearce T. D., Bayo A., Matthews B. C., Löhne T., Wyatt M. C., Ábrahám P., Bonduelle M., Booth M., Cataldi G., Carpenter J. M., Chiang E., Ertel S., Hales A. S., Henning Th., Kóspál Á., Krivov A. V., Luppe P., MacGregor M. A., Marshall J. P., Moór A., Pérez S., Sefilian A. A., Sepulveda A. G., Wilner D. J.
Natura: Artigo
Lingua:Inglês
Pubblicazione: EDP Sciences 2026-01-01
Serie:Astronomy & Astrophysics
Soggetti:
methods: observational
techniques: interferometric
surveys
planet-disk interactions
circumstellar matter
planetary systems
Accesso online:https://www.aanda.org/articles/aa/full_html/2026/01/aa56489-25/aa56489-25.html
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