volume 13, issue S336, P27-32 2017
DOI: 10.1017/s1743921317011632
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Gabriele Surcis, Wouter H. T. Vlemmings, Boy Lankhaar, Huib Jan van Langevelde

Abstract: Through the observations and the analysis of maser polarization it is possible to measure the magnetic field in several astrophysical environments (e.g., star-forming regions, evolved stars). In particular from the linearly and circularly polarized emissions we can determine the orientation and the strength of the magnetic field, respectively. In these proceedings the implications, on observed data, of the new estimation of the Landé g-factors for the CH 3 OH maser are presented. Furthermore, some example of t…

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