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The ALMA survey to Resolve exoKuiper belt Substructures (ARKS)

Context. Dusty discs detected around main-sequence stars are thought to be signs of planetesimal belts in which the dust distribution is shaped by collisional and dynamical processes, including interactions with gas if present. The debris disc around the young A-type star HD 131835 is composed of tw...

Ausführliche Beschreibung

Gespeichert in:
Hauptverfasser: Jankovic M. R., Pawellek N., Zander J., Löhne T., Krivov A. V., Olofsson J., Brennan A., Milli J., Bonduelle M., Wyatt M. C., Sefilian A. A., Pearce T. D., Mac Manamon S., Han Y., Marino S., Matrà L., Moór A., Booth M., Chiang E., Mansell E., Weber P., Hughes A. M., Wilner D. J., Luppe P., Zawadzki B., del Burgo C., Kóspál Á., Pérez S., Carpenter J. M., Henning T.
Format: Artigo
Sprache:Inglês
Veröffentlicht: EDP Sciences 2026-01-01
Schriftenreihe:Astronomy & Astrophysics
Schlagworte:
minor planets, asteroids: general
circumstellar matter
stars: individual: hd 131835
Online-Zugang:https://www.aanda.org/articles/aa/full_html/2026/01/aa56637-25/aa56637-25.html
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