First Year of Postdoctoral Project Successfully Completed
The first year of the project "Investigation of physical mechanisms of mass ejection from young massive stars using CH3OH masers" has concluded with promising results. During this period, 22 star-forming regions were analyzed, with methanol maser emission detected in 13 of them; notably, 5 of these sources are newly discovered.
At the beginning of this year, postdoctoral researcher Artis Aberfelds commenced a 6-month mobility period with the project partner, the Cagliari Astronomical Observatory (OAC). The primary objectives of this residency include: Scientific Publication: Preparing a paper based on the aforementioned research findings. VLA Observations: Planning and processing data from the Very Large Array (VLA) radio telescope network.
Additionally, the researcher has joined the MAGMA (“the role of MAGnetic fields in MAssive star formation”) research project. This collaboration will provide crucial insights into the role of magnetic fields across scales ranging from parsecs to astronomical units

Cartoon of the formation of a young star and distortion of the magnetic field lines (in purple) at different spatial scales, according to a magnetically regulated collapse model.
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