The ALMA-QUARKS Survey: Fibers’ Role in Star Formation Unveiled in an Intermediate-mass Protocluster Region of the Vela D Cloud

Abstract In this paper, we present a detailed analysis of the IRS 17 filament within the intermediate-mass protocluster IRAS 08448-4343 (of ∼10 3 L ⊙ ), using ALMA data from the ATOMS 3 mm and QUARKS 1.3 mm surveys. The IRS 17 filament, which spans ∼54,000 au (0.26 pc) in length and ∼4000 au (0.02 pc) in width, exhibits a complex, multicomponent velocity field and harbors hierarchical substructures. These substructures include three bundles of seven velocity-coherent fibers and 29 dense ( n ∼ 10 8 cm −3 ) condensations. The fibers have a median length of ∼4500 au and a median width of ∼1400 au. Among these fibers, four are identified as “fertile,” each hosting at least three dense condensations, which are regarded as the “seeds” of star formation. While the detected cores are randomly spaced within the IRS 17 filament based on the 3 mm dust continuum image, periodic spacing (∼1600 au) of condensations is observed in the fertile fibers according to the 1.3 mm dust map, consistent with the predictions of linear isothermal cylinder fragmentation models. These findings underscore the crucial role of fibers in star formation and suggest a hierarchical fragmentation process that extends from the filament to the fibers and, ultimately, to the smallest-scale condensations.

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Publication Details

Journal
The Astrophysical Journal
Published
2024-11-26
DOI
https://doi.org/10.3847/1538-4357/ad8919
Citations
5
Primary Topic
Astrophysics and Star Formation Studies
Type
article
Field-Weighted Citation Impact
1.66
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article

The ALMA-QUARKS Survey: Fibers’ Role in Star Formation Unveiled in an Intermediate-mass Protocluster Region of the Vela D Cloud

Dongting Yang, Xiaofeng Mai, Xindi Tang, Tie Liu et al.
5 citations
The Astrophysical Journal
Astrophysics and Star Formation Studies
1.66
article

The ALMA-QUARKS Survey: Fibers’ Role in Star Formation Unveiled in an Intermediate-mass Protocluster Region of the Vela D Cloud

Dongting Yang, Xiaofeng Mai, Xindi Tang, Tie Liu, Jihye Hwang, Patricio Sanhueza, Xunchuan Liu, Suinan Zhang, Shanghuo Li, Fengwei Xu, L. K. Dewangan, Prasanta Gorai, Wenyu Jiao, M. Juvela, Anandmayee Tej, Chang Won Lee, Jinjin Xie, P. F. Goldsmith, Zhiyuan Ren, Pak Shing Li, L. Bronfman, James O. Chibueze, Sheng‐Li Qin, Ken’ichi Tatematsu, Pablo García, Amelia M. Stutz, L. Viktor Tóth, Yichen Zhang, Hongli Liu, Gang Wu, Jinhua He, Swagat Ranjan Das, Guido Garay, Lei Zhu, Siju Zhang
article en
5 citations

Abstract

Abstract In this paper, we present a detailed analysis of the IRS 17 filament within the intermediate-mass protocluster IRAS 08448-4343 (of ∼10 3 L ⊙ ), using ALMA data from the ATOMS 3 mm and QUARKS 1.3 mm surveys. The IRS 17 filament, which spans ∼54,000 au (0.26 pc) in length and ∼4000 au (0.02 pc) in width, exhibits a complex, multicomponent velocity field and harbors hierarchical substructures. These substructures include three bundles of seven velocity-coherent fibers and 29 dense ( n ∼ 10 8 cm −3 ) condensations. The fibers have a median length of ∼4500 au and a median width of ∼1400 au. Among these fibers, four are identified as “fertile,” each hosting at least three dense condensations, which are regarded as the “seeds” of star formation. While the detected cores are randomly spaced within the IRS 17 filament based on the 3 mm dust continuum image, periodic spacing (∼1600 au) of condensations is observed in the fertile fibers according to the 1.3 mm dust map, consistent with the predictions of linear isothermal cylinder fragmentation models. These findings underscore the crucial role of fibers in star formation and suggest a hierarchical fragmentation process that extends from the filament to the fibers and, ultimately, to the smallest-scale condensations.

The Astrophysical JournalVol. 976(2)
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Astrophysics and Star Formation Studies
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