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Magnetic Field in the Proto-Planetary Nebula OH17.7–2.0

Published online by Cambridge University Press:  26 May 2016

Indra Bains ,
Tim Gledhill ,
Jeremy Yates  and
Anita Richards
Indra Bains
Affiliation:
Astronomy Group, Department of Physical Sciences, University of Hertfordshire, College Lane, Hatfield, Hertfordshire, AL10 9AB, UK
Tim Gledhill
Affiliation:
Astronomy Group, Department of Physical Sciences, University of Hertfordshire, College Lane, Hatfield, Hertfordshire, AL10 9AB, UK
Jeremy Yates
Affiliation:
Department of Physics and Astronomy, University College London, Gower Street, London, WC1E 6BT, UK
Anita Richards
Affiliation:
Jodrell Bank Observatory, Department of Physics & Astronomy, University of Manchester, Macclesfield, Cheshire SK11 9DL, UK

Abstract

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We have used radio observations of OH masers in proto-planetary nebula (PPN) candidates to probe the magnetic field structure of these objects. Here we present the first results of our study, concerning the PPN OH17.7–2.0.

Type
Part III: Planetary Nebulae in the Scheme of Stellar Evolution
Information
Symposium - International Astronomical Union , Volume 209: Planetary Nebulae: Their Evolution and Role in the Universe , 2003 , pp. 143 - 144
Copyright
Copyright © Astronomical Society of the Pacific 2003 

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