ATOMS: ALMA three-millimetre observations of massive star-forming regions–XVII. High-mass star-formation through a large-scale collapse in IRAS 15394-5358 Article Swipe
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· 2024
· Open Access
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· DOI: https://doi.org/10.1093/mnras/stae2275
Hub-filament systems are considered as natural sites for high-mass star formation. Kinematic analysis of the surroundings of hub-filaments is essential to better understand high-mass star formation within such systems. In this work, we present a detailed study of the massive Galactic protocluster IRAS 15394$-$5358, using continuum and molecular line data from the ALMA three-millimetre observations of massive star-forming regions (ATOMS) survey. The 3 mm dust continuum map reveals the fragmentation of the massive ($\rm M=843~{\rm M}_{\odot }$) clump into six cores. The core C-1A is the largest (radius = 0.04 pc), the most massive ($\rm M=157~{\rm M}_{\odot }$), and lies within the dense central region, along with two smaller cores ($\rm M=7~and~3~{\rm M}_{\odot }$). The fragmentation process is consistent with the thermal Jeans fragmentation mechanism and virial analysis shows that all the cores have small virial parameter values ($\rm \alpha _{vir}\lt \lt 2$), suggesting that the cores are gravitationally bound. The mass versus radius relation indicates that three cores can potentially form at least a single massive star. The integrated intensity map of $\rm H^{13}CO^{+}$ shows that the massive clump is associated with a hub-filament system, where the central hub is linked with four filaments. A sharp velocity gradient is observed towards the hub, suggesting a global collapse where the filaments are actively feeding the hub. We discuss the role of global collapse and the possible driving mechanisms for the massive star formation activity in the protocluster.
Related Topics
- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.1093/mnras/stae2275
- OA Status
- gold
- Cited By
- 3
- References
- 159
- Related Works
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- OpenAlex ID
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Raw OpenAlex JSON
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https://openalex.org/W4403141291Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.1093/mnras/stae2275Digital Object Identifier
- Title
-
ATOMS: ALMA three-millimetre observations of massive star-forming regions–XVII. High-mass star-formation through a large-scale collapse in IRAS 15394-5358Work title
- Type
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articleOpenAlex work type
- Language
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enPrimary language
- Publication year
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2024Year of publication
- Publication date
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2024-10-03Full publication date if available
- Authors
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Swagat R. Das, Manuel Merello, L. Bronfman, Tie Liu, Guido Garay, Amelia M. Stutz, Diego Mardones, Jianwen Zhou, Patricio Sanhueza, Hongli Liu, Enrique Vázquez-Semadeni, Gilberto C. Gómez, Aina Palau, Anandmayee Tej, Fengwei Xu, Tapas Baug, L. K. Dewangan, Jinhua He, Lei Zhu, Shanghuo Li, M. Juvela, Anindya Saha, Namitha Issac, Jihye Hwang, Hafiz Nazeer, L. Viktor TóthList of authors in order
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https://doi.org/10.1093/mnras/stae2275Publisher landing page
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YesWhether a free full text is available
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goldOpen access status per OpenAlex
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https://doi.org/10.1093/mnras/stae2275Direct OA link when available
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Physics, Astrophysics, High mass, Millimeter, Star (game theory), Star formation, Astronomy, StarsTop concepts (fields/topics) attached by OpenAlex
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3Total citation count in OpenAlex
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2025: 3Per-year citation counts (last 5 years)
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159Number of works referenced by this work
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10Other works algorithmically related by OpenAlex
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