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Polarisation observations of VY Canis Majoris H<sub>2</sub>O 5<sub>32</sub>โ4<sub>41</sub>620.701 GHz maser emission with HIFI
CONTEXT: Water vapour maser emission from evolved oxygen-rich stars remains poorly understood. Additional observations, including polarisation studies and simultaneous observation of different maser transitions may ultimately lead to greater insight. AIMS: We have aimed to elucidate the nature and structure of the VY CMa water vapour masers in part by โฆ