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机译:Population synthesis of binarycarbon-enhanced metal-poor stars
Sterrenkundig Instituut, Universiteit Utrecht, PO Box 80000, 3508 TA Utrecht, The Netherlands;
Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge, CB3 OHA, UK;
stars; carbon – binaries; close – stars; chemically peculiar – Galaxy; halo – Galaxy; stellar content –nuclear reactions; nucleosynthesis; abundances;