Dataset associated with 'Hydrodynamic simulations of mechanical stellar feedback in a molecular cloud formed by thermal instability'
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资源简介：
In the paper, we have used the AMR hydrodynamic code, MG, to perform 3D hydrodynamic simulations with self-gravity of stellar feedback in a spherical clumpy molecular cloud formed through the action of thermal instability. This repository contains the raw data to accompany each figure in this peer-reviewed publication in the Monthly Notices of the Royal Astronomical Society.
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University of Leeds创建时间：
2017-06-02
