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The ALMA survey to Resolve exoKuiper belt Substructures (ARKS)

Context. CO gas is detected in a significant number (~20) of debris discs (exoKuiper belts), but understanding its origin and evolution remains elusive. Crucial pieces of evidence are its mass and spectro-spatial distribution, which are coupled through optical depth and have only been analysed at lo...

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Hoofdauteurs: Mac Manamon S., Matrà L., Marino S., Brennan A., Han Y., Jankovic M. R., Weber P., Bonduelle M., Carpenter J. M., Cataldi G., Hughes A. M., Kóspál A., Marshall J. P., Matthews B. C., Milli J., Moór A., Öberg K., Pérez S., Sefilian A. A., Wilner D. J., Wyatt M. C., Chiang E., Hales A. S., Lovell J. B., Luppe P., MacGregor M. A., Pearce T., Booth M., del Burgo C., Fehr A., Mansell E., Zawadzki B.
Formaat: Artigo
Taal:Inglês
Gepubliceerd in: EDP Sciences 2026-01-01
Reeks:Astronomy & Astrophysics
Onderwerpen:
techniques: interferometric
submillimeter: planetary systems
Online toegang:https://www.aanda.org/articles/aa/full_html/2026/01/aa56605-25/aa56605-25.html
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