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- W1925318785 abstract "We present high signal-to-noise ratio spectrophotometric observations of seven luminous H ii galaxies. The observations have been made with the use of a double-arm spectrograph which provides spectra with a wide wavelength coverage, from 3400 to 10 400 Å free of second-order effects, of exactly the same region as that of a given galaxy. These observations are analysed applying a methodology designed to obtain accurate elemental abundances of oxygen, sulphur, nitrogen, neon, argon and iron in the ionized gas. Four electron temperatures and one electron density are derived from the observed forbidden line ratios using the five-level atom approximation. For our best objects, errors of 1 per cent in te([O iii]), 3 per cent in te([O ii]) and 5 per cent in te([S iii]) are achieved with a resulting accuracy of 7 per cent in total oxygen abundances, O/H." @default.
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- W1925318785 date "2007-12-06" @default.
- W1925318785 modified "2023-10-16" @default.
- W1925318785 title "Precision abundance analysis of bright H ii galaxies" @default.
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- W1925318785 doi "https://doi.org/10.1111/j.1365-2966.2007.12527.x" @default.
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