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Maser Polarization

Published online by Cambridge University Press:  16 July 2018

Gabriele Surcis ,
Wouter H. T. Vlemmings ,
Boy Lankhaar  and
Huib Jan van Langevelde
Gabriele Surcis
Affiliation:
INAF, Osservatorio Astronomico di CagliariVia della Scienza 5, I-09047, Selargius, Italy email: [email protected]
Wouter H. T. Vlemmings
Affiliation:
Department of Space, Earth and Environment, Chalmers University of TechnologyOnsala Space Observatory, 439 92 Onsala, Sweden
Boy Lankhaar
Affiliation:
Department of Space, Earth and Environment, Chalmers University of TechnologyOnsala Space Observatory, 439 92 Onsala, Sweden
Huib Jan van Langevelde
Affiliation:
Joint Institute for VLBI ERICPostbus 2, 7990 AA Dwingeloo, The Netherlands Sterrewacht Leiden, Leiden UniversityPostbus 9513, 2330 RA Leiden, The Netherlands
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Abstract

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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 CH3OH maser are presented. Furthermore, some example of the most recent results achieved in observing the polarized maser emission from several maser species will also be reported.

Keywords

maserspolarizationmagnetic fieldsradiative transfer
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S336: Astrophysical Masers: Unlocking the Mysteries of the Universe , September 2017 , pp. 27 - 32
Copyright
Copyright © International Astronomical Union 2018 

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