Dataset associated with 'A new mechanical stellar wind feedback model for the Rosette Nebula'
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In the paper, we have used the AMR magnetohydrodynamic code, MG, to perform 3D magnetohydrodynamic simulations with self-gravity of stellar feedback in molecular clouds formed through the action of thermal instability in order to reproduce the Rosette Nebula. This repository contains the raw data to accompany various figures in this peer-reviewed publication in the Monthly Notices of the Royal Astronomical Society.
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leeds创建时间：
2018-01-12
