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• W2148292029 startingPage "3161" @default.
• W2148292029 abstract "Zinc is a useful surrogate element for measuring Fe/H as, unlike iron, it is not depleted in the gas phase media. Zn/H and O/Zn ratios have been derived using the [Zn IV] emission line at 3.625um for a sample of nine Galactic planetary nebulae, seven of which are based upon new observations using the VLT. Based on photoionization models, O/O++ is the most reliable ionisation correction factor for zinc that can readily be determined from optical emission lines, with an estimated accuracy of 10% or better for all targets in our sample. The majority of the sample is found to be sub-solar in [Zn/H]. [O/Zn] in half of the sample is found to be consistent with Solar within uncertainties, whereas the remaining half are enhanced in [O/Zn]. [Zn/H] and [O/Zn] as functions of Galactocentric distance have been investigated and there is little evidence to support a trend in either case." @default.
• W2148292029 created "2016-06-24" @default.
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• W2148292029 date "2014-05-30" @default.
• W2148292029 modified "2023-09-23" @default.
• W2148292029 title "Zinc abundances of planetary nebulae" @default.
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• W2148292029 doi "https://doi.org/10.1093/mnras/stu696" @default.
• W2148292029 hasPublicationYear "2014" @default.
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