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Trigonometric Parallaxes of 6.7 GHz Methanol Masers
K. L. J. Rygl, A. Brunthaler, M. J. Reid +3
Emission from the 6.7 GHz methanol maser transition is very strong, is relatively stable, has small internal motions, and is observed toward numerous massive star-forming regions i…
The magnetic field of the evolved star W43A
N. Amiri, W. H. T. Vlemmings, H. J. van Langevelde
The majority of the observed planetary nebulae exhibit elliptical or bipolar structures. Theoretical modeling has indicated that magnetically collimated jets may be responsible for…
Methanol masers probing the ordered magnetic field of W75N
G. Surcis, W. H. T. Vlemmings, R. Dodson +1
The role of magnetic fields during the protostellar phase of high-mass star-formation is a debated topic. In particular, it is still unclear how magnetic fields influence the forma…
The diversity of methanol maser morphologies from VLBI observations
A. Bartkiewicz, M. Szymczak, H. J. van Langevelde +2
We investigate which structures the 6.7 GHz methanol masers trace in the environment of high-mass protostar candidates by observing a homogenous sample of methanol masers selected…