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Magnetic Field in the Proto-Planetary Nebula OH17.7–2.0
Published online by Cambridge University Press: 26 May 2016
Abstract
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.
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- Part III: Planetary Nebulae in the Scheme of Stellar Evolution
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- Copyright © Astronomical Society of the Pacific 2003