ALMA 0.1 pc View of Molecular Clouds Associated with High-mass Protostellar Systems in the Small Magellanic Cloud: Are Low-metallicity Clouds Filamentary or Not?

Filamentary molecular clouds are an essential intermediate stage in the star formation process. To test whether these structures are universal throughout cosmic star formation history, it is crucial to study low-metallicity environments within the Local Group. We present an analysis of Atacama Large...

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Bibliographic Details

Published in:	The Astrophysical Journal
Main Authors:	Kazuki Tokuda, Yuri Kunitoshi, Sarolta Zahorecz, Kei E. I. Tanaka, Itsuki Murakoso, Naoto Harada, Masato I. N. Kobayashi, Tsuyoshi Inoue, Marta Sewiło, Ayu Konishi, Takashi Shimonishi, Yichen Zhang, Yasuo Fukui, Akiko Kawamura, Toshikazu Onishi, Masahiro N. Machida
Format:	Article
Language:	English
Published:	IOP Publishing 2025-01-01
Subjects:	Star formation Protostars Molecular clouds Small Magellanic Cloud Interstellar medium Local Group
Online Access:	https://doi.org/10.3847/1538-4357/ada5f8