Synopsis
Illustrations of Black Hole Eclipse. MPEG These artist's representations, which are not to scale, explain how a supermassive black hole and the hot gas disk around it are eclipsed. The first illustration shows how light from the bright disk surrounding the black hole can directly reach Chandra. The second illustration demonstrates how this light can be blocked by a dense cloud of gas, which causes only reflected light from the disk to reach Chandra. View Still Images
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A note on publication date · savetz · 2025-01-12
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