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Type Ia Supernova Nucleosynthesis: Metallicity-dependent Yields
Published 2023-01-01Get full text
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Tracer Particles for Core-collapse Supernova Nucleosynthesis: The Advantages of Moving Backward
Published 2023-01-01Get full text
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The Dependence of Iron-rich Metal-poor Star Occurrence on Galactic Environment Supports an Origin in Thermonuclear Supernova Nucleosynthesis
Published 2023-01-01“…This difference is thought to demonstrate the importance of thermonuclear supernova nucleosynthesis for the chemical evolution of the Milky Way’s satellite classical dSph galaxies and the Magellanic Clouds. …”
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Ultra-metal-poor Stars: Spectroscopic Determination of Stellar Atmospheric Parameters Using Iron Non-LTE Line Abundances
Published 2018“…Accurate NLTE atmospheric stellar parameters, in particular [Fe/H] being significantly higher, are the first step to eventually providing full NLTE abundance patterns that can be compared with Population III supernova nucleosynthesis yields to derive properties of the first stars. …”
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O, Ne, Mg, and Fe Abundances in Hot X-Ray-emitting Halos of Galaxy Clusters, Groups, and Giant Early-type Galaxies with XMM-Newton RGS Spectroscopy
Published 2023-01-01“…We find that the latest supernova nucleosynthesis models fail to reproduce such a supersolar abundance pattern. …”
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Nucleosynthetic Analysis of Three-dimensional Core-collapse Supernova Simulations
Published 2024-01-01Get full text
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Supernova Dust Evolution Probed by Deep-sea 60Fe Time History
Published 2023-01-01Get full text
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