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Cloud mass function in a gas rich dwarf galaxy

Published online by Cambridge University Press:  26 May 2016

Takayuki Saitou ,
Asao Habe  and
Takashi Okamoto
Takayuki Saitou
Affiliation:
Division of Physics, Graduate School of Science, Hokkaido University, Sapporo 060-0810, Japan
Asao Habe
Affiliation:
Division of Physics, Graduate School of Science, Hokkaido University, Sapporo 060-0810, Japan
Takashi Okamoto
Affiliation:
Yukawa Institute for Theoretical Physics, Kyoto University, Kyoto 606-8502, Japan

Abstract

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We study cloud mass function (here after CMF) obtained in a Grape-SPH simulation of model galaxy. The CMF can be fitted by a simple power law, and its power law index is ∼ −2.0, which closes to the observational results.

Type
Posters
Information
Symposium - International Astronomical Union , Volume 208: Astrophysical Supercomputing using Particle Simulations , 2003 , pp. 441 - 442
Copyright
Copyright © Astronomical Society of the Pacific 2003 

References

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