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dc.contributor.authorKobayashi, Chiaki
dc.contributor.editorDebattista, V P
dc.contributor.editorPopescu, C C
dc.date.accessioned2011-12-20T13:01:14Z
dc.date.available2011-12-20T13:01:14Z
dc.date.issued2010
dc.identifier.citationKobayashi , C 2010 , Chemodynamical Simulations with Variable IMF . in V P Debattista & C C Popescu (eds) , Hunting for the Dark : the Hidden Side of Galaxy Formation . AIP Conf Procs , vol. 1240 , American Institute of Physics (AIP) , MELVILLE , pp. 123-126 , International Conference on Hunting for the Dark: The Hidden Side of Galaxy Formation , Qawra , 19/10/09 . https://doi.org/10.1063/1.3458465
dc.identifier.citationconference
dc.identifier.isbn978-0-7354-0786-2
dc.identifier.otherORCID: /0000-0002-4343-0487/work/62750455
dc.identifier.urihttp://hdl.handle.net/2299/7414
dc.description.abstractUsing self-consistent chemodynamical simulations including star formation, supernova feedback, and chemical enrichment, I show the dependence of the initial mass function (IMF) on cosmic star formation and chemical enrichment histories. The effects of Pop-III IMF can be only seen in the elemental abundance ratios at z greater than or similar to 4 or [Fe/H] less than or similar to - 2. The preferable IMF has a flatter slope in the case of high star formation rate (SFR) and smaller upper-mass (similar to 20M(circle dot)) in the case of low SFR, which is consistent with the observed elemental abundances of dwarf spheroidal galaxies. However, the [alpha/Fe] problem of elliptical galaxies may require other solutions.en
dc.format.extent4
dc.format.extent167839
dc.language.isoeng
dc.publisherAmerican Institute of Physics (AIP)
dc.relation.ispartofHunting for the Dark
dc.relation.ispartofseriesAIP Conf Procs
dc.subjectINITIAL MASS FUNCTION
dc.subjectEVOLUTION
dc.titleChemodynamical Simulations with Variable IMFen
dc.contributor.institutionCentre for Astrophysics Research (CAR)
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
rioxxterms.versionofrecord10.1063/1.3458465
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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