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- W4250847451 abstract "On the diagram (Fe5270, Mg5175) ellipticals and bulges of disk galaxies (from S0 to Sc) maintain a very different position: E's seem to be overabundant in Mg, bulges seem to have a solar ratio Mg/Fe, except several ones who are overabundant in Fe." @default.
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- W4250847451 date "1993-01-01" @default.
- W4250847451 modified "2023-10-18" @default.
- W4250847451 title "On the difference in formation history between bulges and ellipticals" @default.
- W4250847451 cites W2092826856 @default.
- W4250847451 doi "https://doi.org/10.1017/s0074180900123939" @default.
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