How do methanol masers manage to appear in the youngest star vicinities and isolated molecular clumps?

Research output: Contribution to journal › Article › peer-review

Original language	English
Pages (from-to)	81-88
Number of pages	8
Journal	Proceedings of the International Astronomical Union
Volume	3
Issue number	S242
DOIs	https://doi.org/10.1017/S1743921307012616
Publication status	Published - 1 Mar 2007

Catalogs, Evolution, Galaxy: structure, ISM: clouds, Kinematics and dynamics, Masers, Radio lines: ISM, Stars: formation, Structure, Surveys

ID: 8912583