Results 1 to 10 of about 280,504 (183)
Structure and Kinematics of Sh2-138—A Distant Hub-filament System in the Outer Galactic Plane
We present a molecular line study of the Sh2-138 (IRAS 22308+5812) hub-filament system with the aim of investigating its structure and kinematics. Archival CO molecular line data from the Canadian Galactic Plane Survey (CO( J = 1–0)) for the wider region
Kshitiz K. Mallick +4 more
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Magnetic Field of a Ring-like Molecular Cloud
We present a detailed study of the magnetic field structure in the G111 molecular cloud, a ring-like filamentary cloud within the NGC 7538 region. Our analysis combines multiwavelength polarization data and molecular-line observations to investigate the ...
Dana Alina +15 more
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Dust polarization induced by aligned nonspherical grains acts as an important tool to trace the magnetic field ( B -field) morphologies and strengths in molecular clouds and constrain grain properties and their alignment mechanisms.
Saikhom Pravash +7 more
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CMR Exploration. II. Filament Identification with Machine Learning
We adopt magnetohydrodynamic simulations that model the formation of filamentary molecular clouds via the collision-induced magnetic reconnection (CMR) mechanism under varying physical conditions.
Duo Xu +4 more
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Magnetically Aligned Striations in the L914 Filamentary Cloud
We present CO( J = 1–0) multiline observations toward the L914 dark cloud in the vicinity of the Cygnus X region, using the 13.7 m millimeter telescope of the Purple Mountain Observatory.
Li Sun +8 more
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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.
Dongting Yang +34 more
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The study of the volume density distribution of filamentary structures in molecular clouds is crucial for investigating the mechanism of star formation and can reveal the fragmentation process under the effects of gravitational collapse, magnetic fields,
Yapeng Zhang +4 more
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Hub-filament systems (HFSs) are potential sites of massive star formation (MSF). To understand the role of filaments in MSF and the origin of HFSs, we conducted a multiscale and multiwavelength observational investigation of the molecular cloud G321.93–0.
A. K. Maity +7 more
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Large-scale filaments ubiquitously exist in the Galactic interstellar medium, and their radial profiles offer insights into their formation mechanisms. We present a statistical analysis of molecular hydrogen column density (N(H _2 )) and dust temperature
Keyun Su +3 more
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The Structure of an 80 Parsec Long Massive Filament
Using new Institut de Radioastronomie Millimétrique 30 m telescope N _2 H ^+ , C ^18 O J = 1–0 and Atacama Pathfinder Experiment telescope ^13 CO and C ^18 O J = 2–1 maps together with archival far-infrared continuum data, and ^12 CO, and ^13 CO J = 1–
Qian-Ru He +13 more
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