LTE analysis of ALMA data for AG318-c9 yields molecular parameters and spatial maps for three COMs, compared to G31 as a line-identification template for the ALMAGAL survey.
The spatial distribution of dense cores during the evolution of cluster-forming massive clumps
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
astro-ph.GA 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Synthetic Herschel observations from simulations yield 8832 filaments hosting 94% of clumps, with power-law mass and length distributions and a density relation qualitatively matching the Hi-GAL survey.
citing papers explorer
-
ALMAGAL IX. The chemical complexity of AG318.9477-00.1960: A line-identification template for ALMAGAL
LTE analysis of ALMA data for AG318-c9 yields molecular parameters and spatial maps for three COMs, compared to G31 as a line-identification template for the ALMAGAL survey.
-
From filaments to clumps: filament properties with synthetic Herschel observations
Synthetic Herschel observations from simulations yield 8832 filaments hosting 94% of clumps, with power-law mass and length distributions and a density relation qualitatively matching the Hi-GAL survey.