Evolution and Final Fate of Solar Metallicity Stars in the Mass Range 7–15 Msun

Dr. Marco Limongi (INAF-Roma)

13 Giugno 2024
11:30, Aula Piazzi


According to a standard initial mass function, stars in the range 7–12 Msun constitute ∼50% (by number) of the stars more massive than ∼7 Msun, but in spite of this, their evolutionary properties, and in particular their final fate, are still scarcely studied. In this talk, I will present an overview of the evolutionary properties of solar metallicity nonrotating stars in the range 7–15 Msun and their final fate as CO-WD, ONe-WD, Electron Capture Supernovae and Core Collapse Supernovae.

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