Dark Dragon Breaks Magnetic Chain: Dynamical Substructures of IRDC G28.34 Form in Supported Environments Article Swipe
Junhao Liu
,
Qizhou Zhang
,
Yuxin Lin
,
Keping Qiu
,
Patrick M. Koch
,
Hauyu Baobab Liu
,
Zhi‐Yun Li
,
J. M. Girart
,
T. Pillai
,
Shanghuo Li
,
Huei-Ru Vivien Chen
,
Tao-Chung Ching
,
Paul T. P. Ho
,
S. Lai
,
Ramprasad Rao
,
Ya‐Wen Tang
,
Ke Wang
·
YOU?
·
· 2024
· Open Access
·
· DOI: https://doi.org/10.3847/1538-4357/ad3105
YOU?
·
· 2024
· Open Access
·
· DOI: https://doi.org/10.3847/1538-4357/ad3105
We have comprehensively studied the multiscale physical properties of the massive infrared dark cloud G28.34 (the Dragon cloud) with dust polarization and molecular line data from Planck, FCRAO-14 m, James Clerk Maxwell Telescope, and Atacama Large Millimeter/submillimeter Array. We find that the averaged magnetic fields of clumps tend to be either parallel with or perpendicular to the cloud-scale magnetic fields, while the cores in clump MM4 tend to have magnetic fields aligned with the clump fields. Implementing the relative orientation analysis (for magnetic fields, column density gradients, and local gravity), velocity gradient technique, and modified Davis–Chandrasekhar–Fermi analysis, we find that G28.34 is located in a trans-to-sub-Alfvénic environment; the magnetic field is effectively resisting gravitational collapse in large-scale diffuse gas, but is distorted by gravity within the cloud and affected by star formation activities in high-density regions, and the normalized mass-to-flux ratio tends to increase with increasing density and decreasing radius. Considering the thermal, magnetic, and turbulent supports, we find that the environmental gas of G28.34 is in a supervirial (supported) state, the infrared dark clumps may be in a near-equilibrium state, and core MM4-core4 is in a subvirial (gravity-dominant) state. In summary, we suggest that magnetic fields dominate gravity and turbulence in the cloud environment at large scales, resulting in relatively slow cloud formation and evolution processes. Within the cloud, gravity could overwhelm both magnetic fields and turbulence, allowing local dynamical star formation to happen.
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- Type
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- Language
- en
- Landing Page
- https://doi.org/10.3847/1538-4357/ad3105
- https://iopscience.iop.org/article/10.3847/1538-4357/ad3105/pdf
- OA Status
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- Cited By
- 8
- References
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- Related Works
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- OpenAlex ID
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All OpenAlex metadata
Raw OpenAlex JSON
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https://openalex.org/W4395959504Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.3847/1538-4357/ad3105Digital Object Identifier
- Title
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Dark Dragon Breaks Magnetic Chain: Dynamical Substructures of IRDC G28.34 Form in Supported EnvironmentsWork 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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2024-04-29Full publication date if available
- Authors
-
Junhao Liu, Qizhou Zhang, Yuxin Lin, Keping Qiu, Patrick M. Koch, Hauyu Baobab Liu, Zhi‐Yun Li, J. M. Girart, T. Pillai, Shanghuo Li, Huei-Ru Vivien Chen, Tao-Chung Ching, Paul T. P. Ho, S. Lai, Ramprasad Rao, Ya‐Wen Tang, Ke WangList of authors in order
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https://doi.org/10.3847/1538-4357/ad3105Publisher landing page
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https://iopscience.iop.org/article/10.3847/1538-4357/ad3105/pdfDirect link to full text PDF
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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://iopscience.iop.org/article/10.3847/1538-4357/ad3105/pdfDirect OA link when available
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Chain (unit), Evolutionary biology, Physics, Astrobiology, Biology, AstronomyTop concepts (fields/topics) attached by OpenAlex
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8Total citation count in OpenAlex
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2025: 6, 2024: 2Per-year citation counts (last 5 years)
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156Number of works referenced by this work
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10Other works algorithmically related by OpenAlex
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