Aims.We present mm line and continuum observations at high spatial resolution characterizing the physical and chemical properties of the young massive star-forming region IRAS 18182-1433.

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Beuther et al. (Sat,) studied this question.

synapsesocial.com/papers/6a00ef9ff9e1acab462d7745 https://doi.org/https://doi.org/10.1051/0004-6361:20064887

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Also Consider

Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context:

1Testing the Massive Disk Scenario for IRAS 18089−17322005 · 62 citations
2Dust emission from young outflows: The case of L 11572003 · 48 citations
3OH and H<sub>2</sub>O masers in 74 star-forming regions1999 · 99 citations
4The relationship between carbon monoxide abundance and visual extinction in interstellar clouds1982 · 1,051 citations
5A Rotating Disk around a High-Mass Young Star1998 · 133 citations