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Maser Polarization

Date Issued
2018
Author(s)
•
Vlemmings, Wouter H. T.
•
Lankhaar, Boy
•
van Langevelde, Huib Jan
DOI
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 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.
Coverage
Astrophysical Masers: Unlocking the Mysteries of the Universe
All editors
Tarchi, Andrea; Reid, Mark J.; Castangia, Paola
Series
Volume
vol. 13, S336
Start page
27
Conferenece
IAUS 336: Astrophysical Masers: Unlocking the Mysteries of the Universe
Conferenece place
Cagliari, Italia
Conferenece date
4-8 Settembre, 2017
Uri
Url
Issn Identifier
1743-9213
Ads BibCode
2018IAUS..336...27S
Rights
open.access
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