Cambridge University Press, Proceedings of the International Astronomical Union, S287(8), p. 250-251, 2012
DOI: 10.1017/s1743921312007053
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AbstractThe Parkes 64-m telescope was used to study the OH mainline polarisation properties at 1665 and 1667 MHz for a sample of 36 evolved stars, identified by their far-infrared and OH 1612 MHz maser properties as likely post-AGB stars.