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dc.contributor.authorKobayashi, Chiaki
dc.contributor.editorCunha, K
dc.contributor.editorSpite, M
dc.contributor.editorBarbuy, B
dc.date.accessioned2011-12-20T14:01:03Z
dc.date.available2011-12-20T14:01:03Z
dc.date.issued2010
dc.identifier.citationKobayashi , C 2010 , Chemo-dynamical simulations of galaxies . in K Cunha , M Spite & B Barbuy (eds) , Chemical Abundances in the Universe : Connecting First Stars to Planets . Procs of the Int Astronomical Union , vol. 5 , IAU Symposia , vol. 265 , Cambridge University Press , pp. 336-341 , Chemical Abundancies in the Universe: Connecting First Stars to Planets , Rio de Janeiro , Brazil , 10/08/09 . https://doi.org/10.1017/S1743921310000827
dc.identifier.citationconference
dc.identifier.isbn978-0-521-76495-7
dc.identifier.otherORCID: /0000-0002-4343-0487/work/62750437
dc.identifier.urihttp://hdl.handle.net/2299/7416
dc.description.abstractWe 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.en
dc.format.extent6
dc.format.extent1179504
dc.language.isoeng
dc.publisherCambridge University Press
dc.relation.ispartofChemical Abundances in the Universe
dc.relation.ispartofseriesProcs of the Int Astronomical Union
dc.relation.ispartofseriesIAU Symposia
dc.subjectEVOLUTION
dc.titleChemo-dynamical simulations of galaxiesen
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
rioxxterms.versionofrecord10.1017/S1743921310000827
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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