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The evolution of isotope ratios in the Milky Way Galaxy
Chiaki Kobayashi
, Amanda I. Karakas
, Hideyuki Umeda
Centre for Astrophysics Research (CAR)
School of Physics, Engineering & Computer Science
Department of Physics, Astronomy and Mathematics
Research output
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Contribution to journal
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Article
›
peer-review
343
Citations (Scopus)
78
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Dive into the research topics of 'The evolution of isotope ratios in the Milky Way Galaxy'. Together they form a unique fingerprint.
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Keyphrases
Milky Way Galaxy
100%
Isotope Ratio
100%
Solar Neighborhood
80%
Bulge
60%
Halo
40%
Metallicity
40%
α-Fe
40%
Star Formation
40%
Thick Disk
40%
Mn-Fe
40%
Cu-Zn
40%
Asymptotic Giant Branch Stars
40%
Zn-Fe
40%
Supernovae
40%
Core-collapse Supernovae
40%
Chemical Enrichment
40%
Formation Age
20%
Galactic Chemical Evolution
20%
Chemical Evolution
20%
Elemental Abundances
20%
Enrichment Time
20%
Enrichment Efficiency
20%
Stellar Evolution
20%
Low Metallicity
20%
Low-mass
20%
Evolutionary History
20%
C-13
20%
Metal-rich
20%
Early Universe
20%
Type Ia Supernovae
20%
High-alpha
20%
Satellite Galaxies
20%
Evolution Model
20%
Physics
Solar Neighborhood
100%
Milky Way
100%
Metallicity
75%
Asymptotic Giant Branch Stars
50%
Core-Collapse Supernovae
50%
Star Formation
50%
Chemical Enrichment
50%
Chemical Evolution
50%
Supernovae
50%
Early Universe
25%
Elemental Abundance
25%
Stellar Evolution
25%
Type Ia Supernovae
25%
Chemically Peculiar Stars
25%