M31 H II region abundances show a flat oxygen gradient, a steeper nitrogen gradient, and about 0.06 dex intrinsic scatter, with no detected dependence of the CO-to-dust conversion factor on oxygen abundance.
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Cloud-scale elemental abundance variations and the CO-to-dust-mass conversion factor in M31
M31 H II region abundances show a flat oxygen gradient, a steeper nitrogen gradient, and about 0.06 dex intrinsic scatter, with no detected dependence of the CO-to-dust conversion factor on oxygen abundance.