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Filamentary accretion flows in high-mass star-forming clouds
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Filamentary accretion flows in high-mass star-forming clouds
Filamentary accretion flows in high-mass star-forming clouds
Paper

Filamentary accretion flows in high-mass star-forming clouds

2025
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Overview
We quantify the gas flows from a scale of up to several parsecs down to the sub-parsec scale along filamentary structures in the three high-mass star-forming regions G75.78, IRAS21078+5211 and NGC7538 with data obtained from the IRAM 30 m telescope. The analysis is carried out using the surface density derived from 1.2 mm continuum emission and velocity differences estimated from HCO\\(^+\\) and H\\(^13\\)CO\\(^+\\) molecular line data.
Publisher
Cornell University Library, arXiv.org