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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...

    K. Nomoto, K. Maeda, H. Umeda, N. Tominaga, T. Ohkubo, J. Deng… in Cosmic Explosions (2005)