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We report on H$_{2}$O masers around the asymptotic giant branch (AGB) star WX Piscium (WX Psc = IRC +10011), observed with the Japanese VLBI Network (JVN) at three epochs during a span of 2 months. The H$_{2}$O maser spectrum of WX Psc consists of double peaks with a separation of $\sim$ 30 km s$^{-1}$ centered at the systemic velocity of the star. The maser features are found to split roughly in ...

A Pole-on Bipolar Outflow from the AGB Star WX Piscium