Constraining Theories of SiO Maser Polarization: Analysis of a π/2 EVPA Change

T. L. Tobin, A. J. Kemball, M. D. Gray

Research output: Chapter in Book/Conference proceedingConference contributionpeer-review

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Abstract

The full theory of polarized SiO maser emission from the near-circumstellar environment of Asymptotic Giant Branch stars has been the subject of debate, with theories ranging from classical Zeeman origins to predominantly non-Zeeman anisotropic excitation or propagation effects. Features with an internal electric vector position angle (EVPA) rotation of ∼π/2 offer unique constraints on theoretical models. In this work, results are presented for one such feature that persisted across five epochs of SiO ν = 1, J = 1 − 0 VLBA observations of TX Cam. We examine the fit to the predicted dependence of linear polarization and EVPA on angle (θ) between the line of sight and the magnetic field against theoretical models. We also present results on the dependence of mc on θ and their theoretical implications. Finally, we discuss potential causes of the observed differences, and continuing work.
Original languageEnglish
Title of host publicationProceedings of the International Astronomical Union
Subtitle of host publicationVolume 13, Symposium S336 (Astrophysical Masers: Unlocking the Mysteries of the Universe)
PublisherCambridge University Press
Pages53-56
Volume13
EditionS336
DOIs
Publication statusPublished - 16 Jul 2018
EventIAU Symposium 336, Cagliari, Sardinia, Italy - Cagliari, Italy
Duration: 4 Sept 20178 Sept 2017

Publication series

NameProceedings of the International Astronomical Union
PublisherCambridge University Press
ISSN (Print)1743-9213

Conference

ConferenceIAU Symposium 336, Cagliari, Sardinia, Italy
Country/TerritoryItaly
CityCagliari
Period4/09/178/09/17

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