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机译:Abundance patterns in early-type galaxies: is there a "knee" in the Fe/H vs. alpha/Fe relation?
INAF Osservatorio Astrofis Arcetri, I-50125 Florence, Italy;
Ctr Radioastron & Astrofis CRyA, Morelia 58089, Michoacan, Mexico;
UPMC, CNRS, UMR7095, Inst Astrophys Paris, F-75014 Paris, FranceLeibniz Inst Astrophys Potsdam AIP, D-14482 Potsdam, GermanyUniv Sao Paulo, Inst Astron Geofis & Ciencias Atmosfer, BR-05508090 Sao Paulo, Brazil;
galaxies: abundances; galaxies: stellar content; galaxies: elliptical and lenticular; cD;