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- W1679147726 abstract "In previous papers we have published preliminary results on the stellar oxygen-abundance gradient in M33 by using B-type supergiants. In the following study, we include one new B-supergiant and derive effective temperatures and gravities for these stars. Determination of atmospheric parameters is based on analyses of silicon ionisation balance. Detailed non-LTE model atmospheres and non-LTE line formation calculations were used for the abundance determination of Si and O. Careful differential analyses are used to quantify the differences in metal abundances between M33 stars and MK spectral standards in our Galaxy. We compare our results with the abundances expected from studies of H II regions." @default.
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- W1679147726 date "1999-01-01" @default.
- W1679147726 modified "2023-09-26" @default.
- W1679147726 title "Differential Abundances of B-type Supergiants in M33" @default.
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- W1679147726 doi "https://doi.org/10.1017/s0074180900204233" @default.
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