Modeling abundances in galaxies

Chiaki Kobayashi; Philip Taylor

doi:10.1017/S1743921316005160

Modeling abundances in galaxies

Chiaki Kobayashi^*
, Philip Taylor

^*Corresponding author for this work

Research output: Contribution to journal › Article › peer-review

Abstract

We reviewed chemical evolution of galaxies using our cosmological simulations.

Original language	English
Pages (from-to)	246-247
Number of pages	2
Journal	Proceedings of the International Astronomical Union
Volume	11
Issue number	A29B
DOIs	https://doi.org/10.1017/S1743921316005160
Publication status	Published - 2015

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@article{86a9eec97aa54d95b3513e31a4ac799e,

title = "Modeling abundances in galaxies",

abstract = "We reviewed chemical evolution of galaxies using our cosmological simulations.",

keywords = "galaxies: abundances, galaxies: evolution, supernovae: general",

author = "Chiaki Kobayashi and Philip Taylor",

note = "Publisher Copyright: {\textcopyright} International Astronomical Union 2016.",

year = "2015",

doi = "10.1017/S1743921316005160",

language = "English",

volume = "11",

pages = "246--247",

journal = "Proceedings of the International Astronomical Union",

issn = "1743-9213",

publisher = "Cambridge University Press",

number = "A29B",

}

TY - JOUR

T1 - Modeling abundances in galaxies

AU - Kobayashi, Chiaki

AU - Taylor, Philip

N1 - Publisher Copyright: © International Astronomical Union 2016.

PY - 2015

Y1 - 2015

N2 - We reviewed chemical evolution of galaxies using our cosmological simulations.

AB - We reviewed chemical evolution of galaxies using our cosmological simulations.

KW - galaxies: abundances

KW - galaxies: evolution

KW - supernovae: general

UR - https://www.scopus.com/pages/publications/84992560047

U2 - 10.1017/S1743921316005160

DO - 10.1017/S1743921316005160

M3 - Article

SN - 1743-9213

VL - 11

SP - 246

EP - 247

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

IS - A29B

ER -

Modeling abundances in galaxies

Abstract

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