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Symposium - International Astronomical Union
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Symposium - International Astronomical Union
Article . 2003 . Peer-reviewed
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Chemodynamical Evolution of the Milky Way

descriptionPublicationkeyboard_double_arrow_right Article , Other literature type 01 Jan 2003 English Publisher:Cambridge University Press (CUP)Journal:Symposium - International Astronomical Union, volume 208, pages 419-420 (issn: 0074-1809, Copyright policy )
Authors: Ken'ichi Nomoto; Naohito Nakasato; Chiaki Kobayashi;

doi: 10.1017/s0074180900207559

Chemodynamical Evolution of the Milky Way

Abstract

We simulate the chemodynamical evolution of the Milky Way using our GRAPE-SPH code, and reproduce the age-metallicity relation, the [O/Fe]-[Fe/H] relation, and the metallicity distribution.

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citations
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
2
Average
Average
Average
bronze