Recessive
发表于 2025-3-25 06:58:11
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隼鹰
发表于 2025-3-25 11:04:22
Understanding the Enrichment of Heavy Elements by the Chemodynamical Evolution Models of Dwarf Galax
我不死扛
发表于 2025-3-25 13:31:22
Introduction,es. At the time of the big bang, the Universe consists of hydrogen, helium, and lithium. Explosive events such as supernovae and neutron star mergers distribute heavy elements to the interstellar medium. Dense gases containing these elements form stars. Abundances of heavy elements in stars, therefo
演绎
发表于 2025-3-25 18:38:25
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配置
发表于 2025-3-25 22:28:24
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debase
发表于 2025-3-26 00:27:01
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Resistance
发表于 2025-3-26 04:51:54
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Flat-Feet
发表于 2025-3-26 11:47:22
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观察
发表于 2025-3-26 13:38:34
Enrichment of ,-Process Elements in a Cosmological Context,th galaxy formation. In the hierarchical structure formation scenario, galaxies are thought to be formed by clustering of smaller systems. Star-to-star scatters of the ratios of .-process elements in the Milky Way halo should be reflected such process. However, the enrichment of .-process elements i
变化
发表于 2025-3-26 18:27:23
Conclusions and Future Prospects,s. This book aims to understand (1) the contribution of neutron star mergers and supernovae (core-collapse supernovae, hypernovae, electron-capture supernovae, and type Ia supernovae) to the enrichment of heavy elements and (2) the relation between the chemodynamical evolution of galaxies and the ab