Analysis of 3161 molecular clouds reveals oblate shapes aligned with the galactic plane, a flatter velocity dispersion-size relation than Larson's law, strong mass-size correlation, and that 12CO traces diffuse turbulent gas while C18O traces gravity-dominated regions.
Title resolution pending
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
fields
astro-ph.GA 3years
2026 3verdicts
UNVERDICTED 3representative citing papers
Milky Way linear filaments exhibit no strong B-field alignment and bimodal galactic-plane orientations (parallel near midplane, perpendicular far from it), supporting a super-Alfvénic bubbly disk model.
SPH simulations of filament fragmentation indicate isotopic inhomogeneities from 1 pc filaments survive in cores at reduced levels and potentially reach circumstellar disks.
citing papers explorer
-
Statistical Properties of Molecular Clouds in the Milky Way: Insights from Three-Isotopologue CO Observations of the MWISP Project
Analysis of 3161 molecular clouds reveals oblate shapes aligned with the galactic plane, a flatter velocity dispersion-size relation than Larson's law, strong mass-size correlation, and that 12CO traces diffuse turbulent gas while C18O traces gravity-dominated regions.
-
The Milky Way Atlas for Linear Filaments III: Giant filaments and magnetic fields as evidence of a bubbly Galactic disk
Milky Way linear filaments exhibit no strong B-field alignment and bimodal galactic-plane orientations (parallel near midplane, perpendicular far from it), supporting a super-Alfvénic bubbly disk model.
-
Formation of Isotopically Heterogeneous Molecular Cloud Cores in Filamentary Molecular Clouds
SPH simulations of filament fragmentation indicate isotopic inhomogeneities from 1 pc filaments survive in cores at reduced levels and potentially reach circumstellar disks.