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?

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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Detalhes bibliográficos
Principais autores: 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
Formato: Artigo
Idioma:English
Publicado em: IOP Publishing 2025-01-01
coleção:The Astrophysical Journal
Assuntos:
Star formation
Protostars
Molecular clouds
Small Magellanic Cloud
Interstellar medium
Local Group
Acesso em linha:https://doi.org/10.3847/1538-4357/ada5f8

Internet

https://doi.org/10.3847/1538-4357/ada5f8

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