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OH mainline maser polarisation properties of post-AGB stars

Published online by Cambridge University Press:  24 July 2012

Jessica M. Chapman ,
Ioannis Gonidakis ,
Rachel M. Deacon  and
Anne Green
Jessica M. Chapman
Affiliation:
CSIRO Astronomy and Space SciencePO Box 76, Epping, NSW 2122, Australia email: jessica.chapman@csiro.au
Ioannis Gonidakis
Affiliation:
CSIRO Astronomy and Space SciencePO Box 76, Epping, NSW 2122, Australia email: jessica.chapman@csiro.au
Rachel M. Deacon
Affiliation:
University of Sydney, School of Physics NSW 2006, Sydney, Australia
Anne Green
Affiliation:
University of Sydney, School of Physics NSW 2006, Sydney, Australia
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Abstract

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The 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.

Keywords

maserspolarizationstars:AGB and post-AGBradio lines:stars
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S287: Cosmic Masers - from OH to H0 , January 2012 , pp. 250 - 251
Copyright
Copyright © International Astronomical Union 2012

References

Deacon, R. M., Chapman, J. M., & Green, A., 2004, ApJS, 155, 595CrossRefGoogle Scholar
Deacon, R. M., 2006, PhD Thesis, The University of SydneyGoogle Scholar