Abstract
We present measurements of proper motions for circumstellar water maser observations obtained with the VLBA. Results of the observations and modeling indicate that the water masers exist in a kinematically complex region of the circumstellar envelope. A change in position of the maser spots as a function of velocity is discussed.
Original language | English (US) |
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Pages (from-to) | 253-254 |
Journal | International Astronomical Union Colloquium |
Volume | 164 |
DOIs | |
State | Published - Jan 1 1998 |