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特長基線干涉儀

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Image simulation of black hole shadow

圖片來源: Hung-Yi Pu

Image simulation of black hole shadow ("silhouette") images based on a possible accretion flow model.

Three cases of the disk inclination angle 15˚, 45˚, and 85˚ are shown. The observation frequency is 345 GHz. It is expected that black hole shadow can be observed in future mm/sub-mm VLBI observation.