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OH mainline maser polarisation properties of post-AGB stars
Published online by Cambridge University Press: 24 July 2012
Abstract
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.
- 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