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 language | English |
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Title of host publication | In: Procs of Asymmetrical Planetary Nebulae II: From Origins to Microstructures, ASP Conference Series 199 |
Publisher | Astronomical Society of the Pacific |
Pages | 79-82 |
ISBN (Print) | 1-58381-026-9 |
Publication status | Published - 2000 |