Presupernova evolution and explosion of massive stars

Physics

Scientific paper

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Scientific paper

We review our recent progresses on the presupernova evolution of massive stars in the range 11-120 Modot of solar metallicity. Special attention will be devoted to the effect of the mass loss rate during the Wolf-Rayet stages in determining the structure and the physical properties of the star prior the supernova explosion. We also discuss the explosive yields and the initial mass-remnant mass relation in the framework of the kinetic bomb induced explosion and hence the contribution of these stars to the global chemical enrichment of the interstellar medium

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