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- W3123241831 abstract "We combine these new observations with data from the literature to form a sample of dwarf galaxies that all have CO observations and measured oxygen abundances. No known galaxies with 12 + log (O/H) 8.1] metallicities are detected at similar or higher ICO surface brightnesses. The data are consistent with a strong dependence of the ICO/M ≡ XCO conversion factor on ambient metallicity. The strikingly low upper limits on some metal-poor galaxies lead us to predict that the conversion factor is nonlinear, increasing sharply below ~1/10 of the solar metallicity [12 + log (O/H) ≤ 7.9]." @default.
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- W3123241831 date "1998-12-01" @default.
- W3123241831 modified "2023-09-27" @default.
- W3123241831 title "CO Emission in Low-Luminosity, H [CSC]i[/CSC]–rich Galaxies" @default.
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- W3123241831 doi "https://doi.org/10.1086/300655" @default.
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