Radio Observations of Masers in Post-AGB Stars

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dc.creatorDeacon, R. M.
dc.creatorGreen, A. J.
dc.creatorChapman, J. M.
dc.date2003-10-02
dc.date.accessioned2026-07-07T02:09:55Z
dc.date.available2026-07-07T02:09:55Z
dc.descriptionWe present observations of 86 post-Asymptotic Giant Branch (post-AGB) stars of OH maser transitions, taken with the Parkes Telescope between September 2002 and August 2003. Post-AGB stars are the precursors of planetary nebulae, which have a wide range of morphologies that are not well explained. By studying the circumstellar envelopes of post-AGB stars through the masers produced in them, we hope to shed light on the origin of planetary nebula morphologies.
dc.description4 pages + 1 figure. To appear in "Asymmetric Planetary Nebulae III", editors M . Meixner, J.Kastner, B.Balick and N. Soker, ASP conference series
dc.identifierhttps://arxiv.org/abs/astro-ph/0310046
dc.identifierhttp://arxiv.org/abs/astro-ph/0310046
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6616
dc.subjectAstrophysics
dc.titleRadio Observations of Masers in Post-AGB Stars
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