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Chemodynamical simulations of the Milky Way galaxy
Chiaki Kobayashi
, Naohito Nakasato
Centre for Astrophysics Research (CAR)
School of Physics, Engineering & Computer Science
Department of Physics, Astronomy and Mathematics
Research output
:
Contribution to journal
›
Article
›
peer-review
146
Citations (Scopus)
37
Downloads (Pure)
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Keyphrases
α-Fe
100%
Chemo-dynamical
100%
Milky Way Galaxy
100%
Bulge
66%
Mn-Fe
66%
High-alpha
66%
Galaxies
66%
Thin Disk
33%
Halo
33%
Milky Way
33%
Abundance Ratios
33%
Frequency Distribution
33%
Galactic Archaeology
33%
Zinc
33%
Elemental Abundances
33%
Star Formation
33%
Chemical Properties
33%
Thick Disk
33%
Kinematic Properties
33%
Decreasing Trend
33%
HERMES
33%
CuMn
33%
Increasing Trends
33%
Spatial Distribution
33%
Element Distribution
33%
Supernovae
33%
Type Ia Supernovae
33%
Al-Zn-Mg-Cu
33%
Chemical Enrichment
33%
Physics
Disk Stars
100%
Milky Way
100%
Elemental Abundance
50%
Abundance Ratio
50%
Type Ia Supernovae
50%
Frequency Distribution
50%
Star Formation
50%
Chemical Enrichment
50%
Spatial Distribution
50%
Supernovae
50%