Observational tests of SiO maser polarisation models

L. L. Richter, A. J. Kemball, J. L. Jonas

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

SiO masers are often observed in the near-circumstellar envelope of late-type evolved stars. The polarisation of the masers can be used as a probe of the magnetic field in this region, subject to maser polarisation radiative transfer model. Two main maser polarisation models have been developed for the weak Zeeman splitting case applicable to circumstellar SiO masers. Observational tests aimed at discriminating between these models were performed at maser component level, using VLBA observations of v=1 J=1-0, v=2 J=1-0 and v=1 J=2-1 SiO masers towards the high-luminosity source VY CMa.

Original languageEnglish (US)
Title of host publicationCosmic Masers - from OH to H0
EditorsRoy S. Booth, Elizabeth M. L. Humphreys, Wouter H.T. Vlemmings
Pages81-82
Number of pages2
EditionS287
DOIs
StatePublished - Jul 2012

Publication series

NameProceedings of the International Astronomical Union
NumberS287
Volume8
ISSN (Print)1743-9213
ISSN (Electronic)1743-9221

Keywords

  • masers
  • polarization
  • stars: late-type

ASJC Scopus subject areas

  • Medicine (miscellaneous)
  • Astronomy and Astrophysics
  • Nutrition and Dietetics
  • Public Health, Environmental and Occupational Health
  • Space and Planetary Science

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