Origin of the Shell Structure in the Primary Outflow from IRAS 15398−3359

IRAS 15398−3359, a Class 0 protostar in the Lupus I star-forming region, is associated with three generations of outflows. The primary outflow, i.e., the most recent one, shows an internal structure named the “shell structure” in the near-infrared emission map. The shell structure is also seen in th...

詳細記述

書誌詳細
出版年:The Astrophysical Journal
主要な著者: Tomoyuki Hanawa, Yuki Okoda, Yao-Lun Yang, Nami Sakai
フォーマット: 論文
言語:英語
出版事項: IOP Publishing 2025-01-01
主題:
オンライン・アクセス:https://doi.org/10.3847/1538-4357/addac0