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Extragalactic archaeology with the C, N, and O chemical abundances
Fiorenzo Vincenzo,
Chiaki Kobayashi
Centre for Astrophysics Research (CAR)
School of Physics, Engineering & Computer Science
Department of Physics, Astronomy and Mathematics
Research output
:
Contribution to journal
›
Letter
›
peer-review
15
Citations (Scopus)
83
Downloads (Pure)
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Keyphrases
Chemical Abundances
100%
Star Formation History
100%
Archaeology
100%
Supernovae
100%
Disk Galaxies
100%
Galaxy Star Formation
50%
Chemical Evolution
50%
Star-forming
50%
Metallicity
50%
Gas Phase
50%
High-redshift
50%
Star Formation
50%
Almost Flat
50%
James Webb Space Telescope
50%
Asymptotic Giant Branch Stars
50%
Increasing Trends
50%
Galaxies
50%
Cosmological Simulations
50%
Intermediate Mass
50%
Evolution Model
50%
Chemical Enrichment
50%
Interstellar Medium
50%
Physics
Chemical Abundances
100%
Star Formation
100%
Disk Galaxy
66%
Supernovae
66%
James Webb Space Telescope
33%
Asymptotic Giant Branch Stars
33%
Vapor Phase
33%
Interstellar Matter
33%
Metallicity
33%
Chemical Enrichment
33%
Chemical Evolution
33%