Unveiling Fiber Networks and Core Formation in the DR21 South Filament
Kai Yang, Keping Qiu, Xing Pan

TL;DR
This study uses high-resolution millimeter observations to analyze the internal structure, fragmentation, and star-forming activities within the DR21 South Filament, revealing a hierarchical network of fibers and dense cores.
Contribution
It provides detailed characterization of the filament's internal fragmentation, fiber structures, and core properties using high-resolution data, which advances understanding of star formation processes in filaments.
Findings
Most dense cores are gravitationally bound.
H$^{13}$CO$^+$ fibers are more associated with cold cores.
The filament exhibits hierarchical, fiber-based structure.
Abstract
We present high-resolution (1000 AU) 3 mm observations with the NOrthern Extended Millimeter Array toward the DR21 South Filament, aiming to reveal its internal fragmentation and search for deeply embedded star-forming activities. Both the continuum and molecular line emissions align well with the filament axis traced by the low-resolution (18) column density map. The 3 mm continuum, CS (21), and HCO (10) emissions reveal continuous and diffuse structures with measured FWHM widths of 0.054, 0.029, and 0.030 pc, respectively. In contrast, the HCO (10) emission appears more clumpy and localized. The non-thermal motion in the filament is predominantly subsonic to transonic. We detect 13 dense cores in NHD (1), three of which coincide with continuum peaks; virial analysis suggests most are gravitationally bound. Using a…
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Taxonomy
TopicsAstrophysics and Star Formation Studies · Astronomy and Astrophysical Research · Fullerene Chemistry and Applications
