5 Result(s)
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Article
Evidence for p-process nucleosynthesis recorded at the Solar System abundances
Analyzing the Solar System abundance, we have found two universal scaling laws concerning the p- and s-nuclei with the same atomic number. They are evidence of the p-nucleus origin that has been discussed for ...
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Chapter and Conference Paper
Evidence for p-process nucleosynthesis recorded at the Solar System abundances
Analyzing the Solar System abundance, we have found two universal scaling laws concerning the p- and s-nuclei with the same atomic number. They are evidence of the p-nucleus origin that has been discussed for ...
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Chapter and Conference Paper
Nucleosynthesis in Black-Hole-Forming Supernovae
Stars more massive than ∼ 20 − 25 M⨀ form a black hole at the end of their evolution. Stars with non-rotating black holes are likely to collapse “quietly” ejecting a small amount of heavy elements (faint supernov...
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Chapter
Yields from Type Ia Supernovae
Supernovae of both types represent the most important nucleosynthesis contributors to galactic evolution and SNe la represent the major source of Fe-group nuclei. Our theoretical understanding is still burdene...
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Chapter and Conference Paper
Nucleosynthesis in Type II Supernovae and Abundance Trends of Iron-Peak Elements in Metal-Poor Stars
Recent high-resolution abundance surveys show interesting trends of [Cr/Fe], [Mn/Fe], and [Co/Fe] with [Fe/H]. Both [Cr/Fe] and [Mn/Fe] decrease as metallicity declines from [Fe/H] = −2.4 to −4.0, while [Co/Fe...
