IC 5146 dark Streamer: is a first reliable candidate of edge collapse, hub-filament systems, and intertwined sub-filaments?
L. K. Dewangan, N. K. Bhadari, A. Men'shchikov, E. J. Chung, R., Devaraj, C. W. Lee, A. K. Maity, T. Baug

TL;DR
This study analyzes the IC 5146 dark Streamer, revealing intertwined sub-filaments, hub-filament systems, and evidence supporting edge collapse and cloud-cloud collision scenarios in a star-forming region.
Contribution
It provides the first comprehensive observational evidence linking edge collapse, hub-filament systems, and intertwined sub-filaments in a single star-forming filament.
Findings
Discovery of double helix-like intertwined sub-filaments.
Identification of cloud components and their connection via cloud-cloud collision.
Confirmation of edge collapse and hub-filament system presence.
Abstract
The paper presents an analysis of multi-wavelength data of a nearby star-forming site IC 5146 dark Streamer (d 600 pc), which has been treated as a single and long filament, fl. Two hub-filament systems (HFSs) are known toward the eastern and the western ends of fl. Earlier published results favor the simultaneous evidence of HFSs and the end-dominated collapse (EDC) in fl. Herschel column density map (resolution 13.5) reveals two intertwined sub-filaments (i.e., fl-A and fl-B) toward fl, displaying a nearly double helix-like structure. This picture is also supported by the CO(3-2) emission. The scenario "fray and fragment" may explain the origin of intertwined sub-filaments. In the direction of fl, two cloud components around 2 and 4 km s are depicted using the CO(1-0) and CO(1-0) emission, and are connected in velocity space. The HFSs are…
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Taxonomy
TopicsAstrophysics and Star Formation Studies · Astro and Planetary Science · Stellar, planetary, and galactic studies
