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Elemental and isotopic abundances and chemical evolution of galaxies
Chiaki Kobayashi
Centre for Astrophysics Research (CAR)
School of Physics, Engineering & Computer Science
Department of Physics, Astronomy and Mathematics
Research output
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Chapter in Book/Report/Conference proceeding
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Conference contribution
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Dive into the research topics of 'Elemental and isotopic abundances and chemical evolution of galaxies'. Together they form a unique fingerprint.
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Keyphrases
Isotopic Abundance
100%
Elemental Abundances
100%
Galaxy Chemical Evolution
100%
Supernovae
100%
Core-collapse Supernovae
100%
Galaxies
66%
Chemical Enrichment
66%
Damped Lyman-alpha Systems
33%
Stellar Physics
33%
Fainting
33%
18 O
33%
Neutrino Process
33%
Small Systems
33%
Galactic Archaeology
33%
First Stars
33%
Metallicity
33%
Globular Clusters
33%
Relative Contribution
33%
First Galaxies
33%
Low-mass
33%
Chemo-dynamical
33%
Asymptotic Giant Branch Stars
33%
Solar Neighborhood
33%
Isotope Ratio
33%
Galactic Disks
33%
Galactic Bulge
33%
Pair-instability Supernovae
33%
H-relation
33%
Dwarf Spheroidal Galaxies
33%
Carbon-rich
33%
Lambda
33%
Physics
Elemental Abundance
100%
Isotopic Abundance
100%
Galaxy Evolution
100%
Chemical Evolution
100%
Supernovae
100%
Core-Collapse Supernovae
75%
Chemical Enrichment
50%
Asymptotic Giant Branch Stars
25%
Dwarf Spheroidal Galaxies
25%
Population III Stars
25%
Solar Neighborhood
25%
Stellar Astrophysics
25%
Galactic Bulge
25%
Metallicity
25%
Globular Cluster
25%
Damped Lyman-Alpha Systems
25%