PPT-Galactic Evolution Workshop

　 20146466 NAOJ Sachie Arao Yuhri Ishimaru ICU Shinya WanajoRiken Nucleosynthesis of Elements heavier than Fe through 3D inhomogeneous chemical evolution

amp ecsn gyr model ecsn amp model gyr snii dispersion elements trend explain gce inhomogeneous star homogeneous large abundance

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