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...

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Номзүйн дэлгэрэнгүй

Үндсэн зохиолчид:	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.
Формат:	Artigo
Хэл сонгох:	Inglês
Хэвлэсэн:	EDP Sciences 2026-01-01
Цуврал:	Astronomy & Astrophysics
Нөхцлүүд:	minor planets, asteroids: general circumstellar matter stars: individual: hd 131835
Онлайн хандалт:	https://www.aanda.org/articles/aa/full_html/2026/01/aa56637-25/aa56637-25.html
Шошгууд:	Шошго нэмэх Шошго байхгүй, Энэхүү баримтыг шошголох эхний хүн болох!