Emergence of high-mass stars in complex fiber networks (EMERGE) V. From filaments to spheroids: the origin of the hub-filament systems

Autor(en)
A. Hacar, R. Konietzka, D. Seifried, S. E. Clark, A. Socci, F. Bonanomi, A. Burkert, E. Schisano, J. Kainulainen, R. Smith
Abstrakt

Identified as parsec-size, gas clumps at the junction of multiple

filaments, hub-filament systems (HFS) play a crucial role during the

formation of young clusters and high-mass stars. These HFS appear

nevertheless to be detached from most galactic filaments when compared

in the mass-length (M-L) phase-space. We aim to characterize the early

evolution of HFS as part of the filamentary description of the

interstellar medium. Combining previous scaling relations with new

analytic calculations, we created a toy model to explore the different

physical regimes described by the M-L diagram. Despite its simplicity,

our model accurately reproduces several observational properties

reported for filaments and HFS such as their expected typical aspect

ratio ($A$), mean surface density ($\Sigma$), and gas accretion rate

($\dot{m}$). Moreover, this model naturally explains the different mass

and length regimes populated by filaments and HFS, respectively. Our

model predicts a dichotomy between filamentary ($A\geq 3$) and

spheroidal ($A

Organisation(en)
Institut für Astrophysik
Externe Organisation(en)
Harvard-Smithsonian Center for Astrophysics, Universität zu Köln, Stanford University, Ludwig-Maximilians-Universität München, Excellence Cluster ORIGINS, Max-Planck-Institut für extraterrestrische Physik, Istituto di Astrofisica e Planetologia Spaziali , Chalmers University of Technology, University of St. Andrews
Journal
Astronomy & Astrophysics
Band
694
Anzahl der Seiten
17
ISSN
0004-6361
DOI
https://doi.org/10.1051/0004-6361/202450779
Publikationsdatum
11-2024
Peer-reviewed
Ja
ÖFOS 2012
103003 Astronomie, 103004 Astrophysik
Schlagwörter
Link zum Portal
https://ucrisportal.univie.ac.at/de/publications/31c8778a-dd20-4db3-b722-3f0721405d68