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3 He: Does the problem persist?

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Guzman-Ramirez, Lizette; Pineda, J E; Zijlstra, Albert A; Stancliffe, R J; Karakas, Amanda

Description

To understand the chemical evolution of the Galaxy, we need to understand the contribution of planetary nebulae (PNe) in the 3He abundance. 3He abundances have been detected only in a couple of PNe; their abundances are consistent with the standard models

CollectionsANU Research Publications
Date published: 2013
Type: Journal article
URI: http://hdl.handle.net/1885/77600
Source: Monthly Notices of the Royal Astronomical Society
DOI: 10.1093/mnras/stt512

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