The challenge of simultaneously matching the observed diversity of chemical abundance patterns in cosmological hydrodynamical simulations

Physics

• Chemical Abundances 100%
• Chemical Enrichment 50%
• Chemical Evolution 50%
• Hydrodynamical Simulations 100%
• Initial Mass Function 50%
• Massive Star 50%
• Metallicity 50%
• Milky Way 50%
• Milky Way Mass 100%
• Numerical Model 50%
• Stellar Astrophysics 50%
• Vapor Phase 50%

Keyphrases

• Chemical Yield 33%
• Chemo-dynamical 33%
• Enrichment Model 33%
• Galactic Chemical Evolution 33%
• H-plane 33%
• Iron Abundance 33%
• Total Iron 33%
• Yield Table 33%