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Inhomogeneous chemical enrichment in the Galactic Halo
Chiaki Kobayashi
Department of Physics, Astronomy and Mathematics
School of Physics, Engineering & Computer Science
Centre for Astrophysics Research (CAR)
Research output
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peer-review
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Keyphrases
Galactic Halo
100%
Chemical Enrichment
100%
Metal-poor Stars
75%
Galaxies
75%
Intrinsic Variability
50%
Supernovae
50%
Fainting
25%
Mass Explosions
25%
Inhomogeneous Effect
25%
Milky Way
25%
Long Lifetime
25%
Chandrasekhar Mass
25%
Metallicity
25%
Elemental Abundances
25%
Local Variation
25%
Low Metallicity
25%
Carbon Enhancement
25%
Star Formation
25%
Star-star
25%
Low-mass
25%
Radial Migration
25%
Chemo-dynamical
25%
Asymptotic Giant Branch Stars
25%
Early Universe
25%
Type Ia Supernovae
25%
Early Metals
25%
Nucleosynthesis
25%
Satellite Galaxies
25%
Dwarf Spheroidal Galaxies
25%
Neutron Star Mergers
25%
Knee
25%
Physics
Galactic Halos
100%
Chemical Enrichment
100%
Metallicity
50%
Supernovae
50%
Early Universe
25%
Elemental Abundance
25%
Asymptotic Giant Branch Stars
25%
Nuclear Fusion
25%
Dwarf Spheroidal Galaxies
25%
Type Ia Supernovae
25%
Milky Way
25%
Neutron Star Mergers
25%
Star Formation
25%