Is the Outflow from RT Vir Bipolar or Rotating

J.A. Yates, A.M.S. Richards, T. Gledhill, I. Bains

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

    28 Downloads (Pure)

    Abstract

    We present high angular resolution observations of H2O maser proper motions in the circumstellar envelope of the semi-regular variable RT Vir. The MERLIN observations, at 12-mas angular resolution, were used to map H2O maser emission at ~2 week intervals over 10 weeks in 1996, during which period the brightness distribution changed markedly.
    Original languageEnglish
    Title of host publicationIn: Procs of Asymmetrical Planetary Nebulae II: From Origins to Microstructures, ASP Conference Series 199
    PublisherAstronomical Society of the Pacific
    Pages79-82
    ISBN (Print)1-58381-026-9
    Publication statusPublished - 2000

    Fingerprint

    Dive into the research topics of 'Is the Outflow from RT Vir Bipolar or Rotating'. Together they form a unique fingerprint.

    Cite this