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Rapid Chemical Enrichment by Intermittent Star Formation in GN-z11
Chiaki Kobayashi
, Andrea Ferrara
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
›
Article
›
peer-review
62
Citations (Scopus)
40
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Dive into the research topics of 'Rapid Chemical Enrichment by Intermittent Star Formation in GN-z11'. Together they form a unique fingerprint.
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Keyphrases
Star Formation
100%
Chemical Enrichment
100%
Galaxies
50%
Nuclear Astrophysics
50%
James Webb Space Telescope
50%
Star Formation History
50%
Nucleosynthesis
50%
Massive Stars
50%
Starburst
50%
Evolutionary Model
50%
Telescope Observations
50%
Chemical Evolution
50%
Quiescent Phase
50%
Elemental Abundances
50%
Wolf-Rayet Stars
50%
Initial Mass Function
50%
Burst Model
50%
Stellar Astrophysics
50%
Pre-enrichment
50%
Isotope 13C
50%
Pair-instability Supernovae
50%
Physics
Star Formation
100%
Chemical Enrichment
100%
James Webb Space Telescope
33%
Nuclear Fusion
33%
Chemical Evolution
33%
Nuclear Astrophysics
33%
Supernovae
33%
Elemental Abundance
33%
Wolf Rayet Star
33%
Initial Mass Function
33%
Stellar Astronomy
33%
Massive Star
33%
Nitrogen
33%
Earth and Planetary Sciences
Star Formation
100%
State of the Art
33%
Nuclear Fusion
33%
Massive Star
33%
Supernovae
33%
Chemical Element
33%
Chemical Evolution
33%
James Webb Space Telescope
33%
Astrophysics
33%
Nitrogen
33%
Wolf Rayet Star
33%