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Maser Polarization

Published online by Cambridge University Press:  16 July 2018

Gabriele Surcis
Affiliation:
INAF, Osservatorio Astronomico di CagliariVia della Scienza 5, I-09047, Selargius, Italy email: surcis@oa-cagliari.inaf.it
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.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2018 

References

Assaf, K. A., Diamond, P. J., Richards, A. M. S., & Gray, M. D., 2013, MNRAS, 431, 1077CrossRefGoogle Scholar
Herpin, F., Baudry, A., Thum, C., Morris, D., & Wiesemeyer, H., 2006, A&A, 450, 667Google Scholar
Lankhaar, B., Groenenboom, G., & van der Avoird, A., 2016, J. Chem. Phys., 145, 24CrossRefGoogle Scholar
Lankhaar, B., Vlemmings, W. H. T., Surcis, G., van Langevelde, H. J., Groenenboom, G., & van der Avoird, A., 2017, Nature Astronomy, 2, 145LCrossRefGoogle Scholar
Nedoluha, G. E. & Watson, W. D., 1992, ApJ, 384, 185CrossRefGoogle Scholar
Peréz-Sánchez, A. F. & Vlemmings, W. H. T., 2013, A&A, 551A, 15Google Scholar
Richter, L., Kemball, A., & Jonas, J., 2016, MNRAS, 461, 2309CrossRefGoogle Scholar
Surcis, G., Vlemmings, W. H. T., van Langevelde, H. J., Goddi, C., Torrelles, J. M., Cantó, J., Curiel, S., Kim, S.-W., & Kim, J.-S., 2014, A&A, 565, L8Google Scholar
Surcis, G., Vlemmings, W. H. T., van Langevelde, H. J., Hutawarakorn Kramer, B., Bartkiewicz, A., & Blasi, M. G., 2015, A&A, 578, 102Google Scholar
Vlemmings, W. H. T., Diamond, P. J., van Langevelde, H. J., & Torrelles, J. M., 2006, A&A, 448, 597Google Scholar
Vlemmings, W. H. T., Surcis, G., Torstensson, K. J. E., & van Langevelde, H. J., 2010, MNRAS, 404, 134Google Scholar
Vlemmings, W. H. T., Torres, R. M., & Dodson, R., 2011, A&A, 529, 95Google Scholar
Vlemmings, W. H. T., Khouri, T., Martí-Vidal, I., Tafoya, D., Baudry, A., Etoka, S., Humphreys, E. M. L., Jones, T. J., Kemball, A., O'Gorman, E., Peréz-Sánchez, A. F., & Richards, A., 2017, A&A, 603, 92Google Scholar