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Showing 1 to 2 of 2 for “"SiO masers"”.

  1. The Structure and Polarization Properties of the SiO Masers in the Extended Atmosphere of R Aquarii

    Silicon monoxide (SiO) maser emission has been observed towards many late-type stars. The conditions necessary for the formation of SiO masers dictate that they be produced in a region which is inside the silicate dust formation point close to the surface of the star. Very Long Baseline …

    vt Repository record for The Structure and Polarization Properties of the SiO Masers in the Extended Atmosphere of R Aquarii (opens in a new tab)

  2. Observational and theoretical studies of SiO maser polarization toward late-type evolved stars: Insights from EVPA reversal features

    … mechanisms responsible for the polarization of SiO masers toward late-type evolved stars continue to be a subject of debate. Possible primary sources include the local magnetic field or anisotropic pumping, while additional polarization may arise due to conversion from linear to circular modes …

    uiuc Repository record for Observational and theoretical studies of SiO maser polarization toward late-type evolved stars: Insights from EVPA reversal features (opens in a new tab)