Is the Outflow from RT Vir Bipolar or Rotating

Yates, J.A., Richards, A.M.S., Gledhill, T. and Bains, I. (2000) Is the Outflow from RT Vir Bipolar or Rotating. In: In: Procs of Asymmetrical Planetary Nebulae II: From Origins to Microstructures, ASP Conference Series 199 :. Astronomical Society of the Pacific, pp. 79-82. ISBN 1-58381-026-9
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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.
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Additional information Original paper can be found at: http://www.astrosociety.org/pubs/cs/195-221.html--Copyright Astronomical Society of the Pacific
Date Deposited 15 May 2025 16:18
Last Modified 30 May 2025 23:08

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