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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Bibliografiske detaljer

Principais autores:	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.
Format:	Artigo
Sprog:	Inglês
Udgivet:	EDP Sciences 2026-01-01
Serier:	Astronomy & Astrophysics
Fag:	techniques: interferometric submillimeter: planetary systems
Online adgang:	https://www.aanda.org/articles/aa/full_html/2026/01/aa56605-25/aa56605-25.html
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