Masers in star forming regions
Anna Bartkiewicz (1), Huib Jan van Langevelde (2, 3) ((1) Torun, Centre for Astronomy, Poland, (2) JIVE, Dwingeloo (3) Sterrewacht Leiden,, Leiden University, the Netherlands)
TL;DR
This paper reviews recent observational and theoretical progress on maser emissions in star forming regions, highlighting their importance in understanding the kinematics and physical conditions near young stars.
Contribution
It provides an updated summary of advances in maser studies related to star formation since the last IAU Symposium 242.
Findings
Enhanced understanding of maser kinematics near young stars
Improved models of physical conditions in star forming regions
Recent observational techniques for maser detection
Abstract
Maser emission plays an important role as a tool in star formation studies. It is widely used for deriving kinematics, as well as the physical conditions of different structures, hidden in the dense environment very close to the young stars, for example associated with the onset of jets and outflows. We will summarize the recent observational and theoretical progress on this topic since the last maser symposium: the IAU Symposium 242 in Alice Springs.
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