Semi-Analytic Models on the Molecular and Neutral Gas in Galaxies

Details Semi-Analytic Models on the Molecular and Neutral Gas in Galaxies Semi-Analytic Models on the Molecular and Neutral Gas in Galaxies

2010-03-24

arxiv.org/abs/1003.4581v2

Astronomy and Astrophysics

Astrophysics

Cosmology and Extragalactic Astrophysics

This paper has been withdrawn by the author due to not contain sufficient content to be understood properly.

Scientific paper

We introduced a semi-analytic model to study the detail of radial related processes on galaxy disks. Based on this recipe, we can calculate neutral and molecular gas in interstellar medium, and include the molecular phase into star formation recipes. From our model, we reproduced the radial surface density profiles and mass functions shown in the observational results. We can also give some predictions and explanations to the scale relations of neutral and molecular gas in disk galaxies.

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