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Astrometry of circumstellar masers

The circumstellar masers around evolved stars offer an interesting possibility to measure stellar parameters through VLBI astrometry. In this paper the application of this technique is discussed, including the accuracy and the uncertainties of the method. The different maser species (OH, H_2O, SiO) have slightly different characteristics and applications. This paper does not concern astrometry of maser spots to study the kinematics of the envelope, but concentrates on attempting to measure the motion of the underlying star.

preprint2002arXivOpen access
H. J. van LangeveldeW. H. T. Vlemmings
astro-ph
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Open access2 authors1 topic
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H. J. van LangeveldeW. H. T. Vlemmings

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