Magnetic fields in the envelopes of late-type stars: circular polarization of H2O masers.

W. H. T. Vlemmings, P. J. Diamond, H. J. van Langevelde

    Research output: Contribution to journalArticlepeer-review

    Abstract

    We present the first circular polarization measurements of circumstellar H2O masers around a sample of late-type stars. These observations are used to obtain the magnetic field strength in the H2O maser region with both an LTE and non-LTE anal. We find fields from a few hundred milliGauss up to a few Gauss, indicating a solar-type r-2 dependence of the magnetic field on the distance. No linear polarization is detected to less than 1%. [on SciFinder (R)]
    Original languageEnglish
    Pages (from-to)291-294
    JournalAstrophysics and Space Science Library
    Volume283
    DOIs
    Publication statusPublished - 2003

    Keywords

    • Masers (cosmic; magnetic fields in envelopes of late-type stars measured by circular polarization of H2O masers); Circumstellar shells; Late-type stars (magnetic fields in envelopes of late-type stars measured by circular polarization of H2O masers); Magnetic field (stellar; magnetic fields in envelopes of late-type stars measured by circular polarization of H2O masers)

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