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The Structure and Kinematics of the ISM in Simulated Star-forming Galaxies

Published online by Cambridge University Press:  09 February 2015

Junichi Baba ,
Kana Morokuma-Matsui  and
Takayuki R. Saitoh
Junichi Baba
Affiliation:
Earth-Life Science Institute (ELSI), Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro, Tokyo152–8551 email: babajn@elsi.jp; babajn2000@gmail.com
Kana Morokuma-Matsui
Affiliation:
Nobeyama Radio Observatory, National Astronomical Observatory of Japan, Minamimaki, Minamisaku, Nagano, 384-1305, Japan
Takayuki R. Saitoh
Affiliation:
Earth-Life Science Institute (ELSI), Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro, Tokyo152–8551 email: babajn@elsi.jp; babajn2000@gmail.com
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Abstract

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We performed 3D N-body/hydrodynamic simulations of local and high-z (z ∼ 2) star-forming galaxies (SFGs) to investigate the structure and kinematic properties of the different ISM phases (i.e., ionized, atomic, and molecular gases). We took into account, for the first time, a fully non-equilibrium radiative cooling by solving the non-equilibrium chemistries of atoms (H, He, C and O) and molecules (H2 and CO), as well as radiative heating, star formation, heating by HII region and supernova explosions.

References

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