研究成果藝廊 > 高能天文物理
研究成果藝廊
高能天文物理
Hypernovae and GRB |
圖片來源: Ke-Jung Chen
![]() The image shows the density distribution of a hypernova. An energetic explosion driven by both jets and disk winds leads to a large scale asymmetry in SN ejecta.
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