Binaries, galactic chemical evolution an
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D. Vanbeveren; E. De Donder
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Article
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2010
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Elsevier Science
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English
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Low metallicity very massive stars with an initial mass between 140 M and 260 M can be subdivided into two groups: those between 140 M and 200 M which produce a relatively small amount of Fe, and those with a mass between 200 M and 260 M where the Fe-yield ejected during the supernova explosion is e