@inproceedings{96675dfb7a90431492275618634b9e5d,
title = "Chemo-dynamical simulations of galaxies",
abstract = "We simulate the formation and evolution of galaxies with a self-consistent 3D hydrodynamical model including star formation, supernova feedback, and chemical enrichment. Hypernova feedback plays an essential role not only in solving the [Zn/Fe] problem, but also reproducing the cosmic star formation rate history and the mass-metallicity relations. In the Milky-Way type galaxy, the star formation history, and thus the kinematics and chemical abundances are different in bulge, disk, and thick disk.",
keywords = "EVOLUTION",
author = "Chiaki Kobayashi",
year = "2010",
doi = "10.1017/S1743921310000827",
language = "English",
isbn = "978-0-521-76495-7",
series = "Procs of the Int Astronomical Union",
publisher = "Cambridge University Press",
pages = "336--341",
editor = "K Cunha and M Spite and B Barbuy",
booktitle = "Chemical Abundances in the Universe",
address = "United Kingdom",
note = "Chemical Abundancies in the Universe: Connecting First Stars to Planets ; Conference date: 10-08-2009 Through 14-08-2009",
}