The hierarchical fragmentation of filaments and the role of sub-filaments
arXiv:2007.15358 · doi:10.1093/mnras/staa2298
Abstract
Recent observations have revealed the presence of small fibres or sub-filaments within larger filaments. We present a numerical fragmentation study of fibrous filaments investigating the link between cores and sub-filaments using hydrodynamical simulations performed with the moving-mesh code Arepo. Our study suggests that cores form in two environments: (i) as isolated cores, or small chains of cores, on a single sub-filament, or (ii) as an ensemble of cores located at the junction of sub-filaments. We term these isolated and hub cores respectively. We show that these core populations are statistically different from each other. Hub cores have a greater mean mass than isolated cores, and the mass distribution of hub cores is significantly wider than isolated cores. This fragmentation is reminiscent of parsec-scale hub-filament systems, showing that the combination of turbulence and gravity leads to similar fragmentation signatures on multiple scales, even within filaments. Moreover, the fact that fragmentation proceeds through sub-filaments suggests that there exists no characteristic fragmentation length-scale between cores. This is in opposition to earlier theoretical works studying fibre-less filaments which suggest a strong tendency towards the formation of quasi-periodically spaced cores, but in better agreement with observations. We also show tentative signs that global collapse of filaments preferentially form cores at both filament ends, which are more massive and dense than other cores.
arXiv commentAccepted in MNRAS. 13 pages and 13 figures, 8 page appendix and 7 figures
References in corpus (46)
- scikit-image: Image processing in Python
- E pur si muove: Galiliean-invariant cosmological hydrodynamical simulations on a moving mesh
- From filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt survey
- Characterizing interstellar filaments with Herschel in IC5146
- The persistent cosmic web and its filamentary structure I: Theory and implementation
- Filamentary structure of star-forming complexes
- Cores, filaments, and bundles: hierarchical core formation in the L1495/B213 Taurus region
- Global collapse of molecular clouds as a formation mechanism for the most massive stars
- The SILCC (SImulating the LifeCycle of molecular Clouds) project: I. Chemical evolution of the supernova-driven ISM
- Cluster-formation in the Rosette molecular cloud at the junctions of filaments
- SDC13 infrared dark clouds: Longitudinally collapsing filaments?
- An ALMA study of the Orion Integral Filament: I. Evidence for narrow fibers in a massive cloud
- From Filamentary Networks to Dense Cores in Molecular Clouds: Toward a New Paradigm for Star Formation
- Characterizing the properties of nearby molecular filaments observed with Herschel
- The "Nessie" Nebula: Cluster Formation in a Filamentary Infrared Dark Cloud
- A census of dense cores in the Aquila cloud complex: SPIRE/PACS observations from the Herschel Gould Belt survey
- Chains of dense cores in the Taurus L1495/B213 complex
- Physical properties of interstellar filaments
- Formation and evolution of interstellar filaments; Hints from velocity dispersion measurements
- The identification of filaments on far infrared and submillimiter images. Morphology, physical conditions and relation with star formation of filamentary structure
- On the nature of star-forming filaments: II. Sub-filaments and velocities
- A census of dense cores in the Taurus L1495 cloud from the Herschel Gould Belt Survey
- SILCC-Zoom: The dynamical and chemical evolution of molecular clouds
- Gravity drives the evolution of infrared dark hubs: JVLA observations of SDC13
- Dynamics of cluster-forming hub-filament systems: The case of the high-mass star-forming complex Monoceros R2
- Unveiling a network of parallel filaments in the Infrared Dark Cloud G14.225-0.506
- Filamentary fragmentation in a turbulent medium
- ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions -- I. Survey description and a first look at G9.62+0.19
- The Herschel view of the dense core population in the Ophiuchus molecular cloud
- Resolving the fragmentation of high line-mass filaments with ALMA: the integral shaped filament in Orion A
- VLA observations of ammonia in high-mass star formation regions
- Synthetic CO observations of fibrous filaments: the problems of mapping from PPV to PPP
- Gravitational fragmentation caught in the act: the filamentary Musca molecular cloud
- Filament Fragmentation in High-Mass Star Formation
- The CARMA-NRO Orion Survey: The filamentary structure as seen in CO emission
- Investigating the structure and fragmentation of a highly filamentary IRDC
- Perturbation growth in accreting filaments
- Investigating the Global Collapse of Filaments Using Smoothed Particle Hydrodynamics
- Morphology and Kinematics of Filaments in the Serpens and Perseus Molecular Clouds
- Two-level hierarchical fragmentation in the Orion Molecular Cloud 1 northern filament
- The Clustering Evolution of Distant Red Galaxies in the GOODS-MUSIC Sample
- Are fibres in molecular cloud filaments real objects?
- Structure and stability in TMC-1: analysis of NH molecular line and Herschel continuum data
- Observational signatures of end-dominated collapse in the S242 filamentary structure
- Edge collapse and subsequent longitudinal accretion in Filament S242
- Determining the presence of characteristic fragmentation length-scales in filaments
Cited by in corpus (14)
- LOC program for line radiative transfer
- A Morphological Classification of 18190 Molecular Clouds Identified in CO Data from the MWISP Survey
- Simultaneous evidence of edge collapse and hub-filament configurations: A rare case study of a Giant Molecular Filament G45.3+0.1
- Supervised machine learning on Galactic filaments Revealing the filamentary structure of the Galactic interstellar medium
- The SEDIGISM survey: Molecular cloud morphology. I. Classification and star formation
- ALMA Fragmented Source Catalogue in Orion (FraSCO) I. Outflow interaction within an embedded cluster in OMC-2/FIR3, FIR4, and FIR5
- AFGL 5180 and AFGL 6366S: sites of hub-filament systems at the opposite edges of a filamentary cloud
- Filling in the Gaps: Can Gravitationally Unstable Discs Form the Seeds of Gas Giant Planets?
- RJ-plots: An improved method to classify structures objectively
- A Herschel study of G214.5-1.8: a young, cold and quiescent giant molecular filament on the shell of a HI superbubble
- Star Cluster Formation in Clouds with Externally Driven Turbulence
- Investigations of MWISP Filaments. I. Filament Identification and Analysis Algorithms, and Source Catalogue
- The SARAO MeerKAT Galactic Plane Survey filamentary source catalogue
- SiO emission in the filamentary Infrared Dark Cloud G035.39-00.33: An ALMA view