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- W763982274 abstract "A method for obtaining the C/O elemental abundance ratio for high excitation H II regions is discussed. This is applied to rederive C/O for the Orion Nebula from IUE observations using improved atomic data and extinction corrections. It is found that C/H is 20 to 40% lower than previously determined. When recombinations contribute importantly to (O II) 2470 and 7325 A emission, use of these lines for assessing the O(+) ionic abundance with the so-called empirical method is inadvisable." @default.
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- W763982274 date "1986-09-01" @default.
- W763982274 modified "2023-09-27" @default.
- W763982274 title "Elemental abundance determination in gaseous nebulae from IUE lines" @default.
- W763982274 hasPublicationYear "1986" @default.
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