The ALMA survey to Resolve exoKuiper belt Substructures (ARKS)

Context. CO gas has been detected in ~20 debris discs, typically classified as CO-poor or CO-rich. We present observations of the CO-rich HD 121617 debris disc as part of the ALMA survey to Resolve exoKuiper belt Substructures (ARKS). Aims. We model local CO line profiles in the HD 121617 debris dis...

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Hlavní autoři:	Brennan A., Matrà L., Mac Manamon S., Marino S., Cataldi G., Hughes A. M., Weber P., Han Y., Marshall J. P., Zawadzki B., Luppe P., Sefilian A. A., Moór A., MacGregor M. A., Lovell J. B., Kóspál A., Bonduelle M., Mansell E., Wyatt M. C., Pearce T. D., Carpenter J. M., Wilner D. J., del Burgo C., Pérez S., Henning T., Milli J., Chiang E.
Médium:	Artigo
Jazyk:	Inglês
Vydáno:	EDP Sciences 2026-01-01
Edice:	Astronomy & Astrophysics
Témata:	radiative transfer methods: observational techniques: interferometric circumstellar matter planetary systems
On-line přístup:	https://www.aanda.org/articles/aa/full_html/2026/01/aa56566-25/aa56566-25.html
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