University of Hertfordshire

By the same authors

Chemo-dynamical simulations of galaxies

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Documents

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Original languageEnglish
Title of host publicationChemical Abundances in the Universe
Subtitle of host publicationConnecting First Stars to Planets
EditorsK Cunha, M Spite, B Barbuy
PublisherCambridge University Press
Pages336-341
Number of pages6
ISBN (Print)978-0-521-76495-7
DOIs
Publication statusPublished - 2010
EventChemical Abundancies in the Universe: Connecting First Stars to Planets - Rio de Janeiro, Brazil
Duration: 10 Aug 200914 Aug 2009

Publication series

NameProcs of the Int Astronomical Union
PublisherCambridge University Press
Volume5
NameIAU Symposia
PublisherCambridge University Press
Volume265

Conference

ConferenceChemical Abundancies in the Universe: Connecting First Stars to Planets
Country/TerritoryBrazil
CityRio de Janeiro
Period10/08/0914/08/09

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.

ID: 494105