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- W1965333669 abstract "Oxygen, helium, and neon abundances are derived from image-dissector scanner observations of 10 emission-line dwarf galaxies. The n(0)/n(H) ratios range from 0.025 to 0.5 the solar value, with the expected anticorrelation with gas temperature. Assuming that n(Ne/sup + +/)/n(O/sup + +/)roughly-equaln(Ne)/n(O), we find a value of 0.23 for this ratio, which is about 50% higher than the values quoted for Orion and the Magellanic Clouds. The mean ratio of n(He/sup +/, He/sup + +/)/n(H/sup +/) is 0.082 +- 0.007 for the five best observed galaxies: we do not detect any correlation of this ratio with the oxygen abundance. Reasons are given to refrain from deriving nitrogen abundances for these galaxies. It seems likely that the underlying continua in these galaxies come predominantly from mixtures of O-type stars and moderately hot giants and supergiants." @default.
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- W1965333669 date "1981-01-01" @default.
- W1965333669 modified "2023-09-26" @default.
- W1965333669 title "Spectroscopic observations of 10 emission-line dwarf galaxies" @default.
- W1965333669 doi "https://doi.org/10.1086/158575" @default.
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