Published in

Cambridge University Press, Proceedings of the International Astronomical Union, S287(8), p. 250-251, 2012

DOI: 10.1017/s1743921312007053

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OH mainline maser polarisation properties of post-AGB stars

Journal article published in 2012 by Jessica M. Chapman, Ioannis Gonidakis, Rachel M. Deacon ORCID, Anne Green
This paper is available in a repository.
This paper is available in a repository.

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Data provided by SHERPA/RoMEO

Abstract

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.