Colliding Stellar Winds Structure and X-ray Emission
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In the paper, we have used a hydrodynamics code to perform 2D axisymmetric simulations of the wind-wind collision in a massive star binary system. 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:
2018-07-31



