研究成果藝廊 > 高能天文物理
研究成果藝廊
高能天文物理
3D radiation hydrodynamical simulation of Colliding Shells |
圖片來源: Ke-Jung Chen
The image shows the density structure of colliding shells ejected by a massive star before it dies. Such collisions can easily convert the kinetic energy of ejecta into thermal radiation.
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