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ALMA-IMF

We characterize kinematic processes in the G012.80 protocluster. We primarily focused on the N2H+(1−0) emission to trace the dense and cold gas. Additionally, we used complementary lines such as DCN(3-2), H41α, C18O(2−1), and SiO(5−4), as well as continuum maps. We performed a N2H+ hyperfine spectra...

Бүрэн тодорхойлолт

-д хадгалсан:
Үндсэн зохиолчид: Salinas J., Stutz A. M., Álvarez-Gutiérrez R. H., Sandoval-Garrido N. A., Louvet F., Galván-Madrid R., Motte F., Armante M., Csengeri T., Braine J., Ginsburg A., Valeille-Manet M., Bronfman L., Sanhueza P., Díaz D., Busquet G., Koley A., Bonfand M., Fernández-López M., Gusdorf A., Castro-Toledo N., Veyry R., Bernal-Mesina G.
Формат: Artigo
Хэл сонгох:Inglês
Хэвлэсэн: EDP Sciences 2026-07-01
Цуврал:Astronomy & Astrophysics
Нөхцлүүд:
evolution
hii regions
ism: kinematics and dynamics
Онлайн хандалт:https://www.aanda.org/articles/aa/full_html/2026/07/aa57551-25/aa57551-25.html
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