The next step is to examine these subtle
The next step is to examine these subtle
differences more closely and see whether they hold clues to discern a black hole's orientation. Eventually, our future measurements of black holes could be even more accurate.
More information: Ji-Jia Tang et al, Universality in the random walk structure function of luminous quasi-stellar objects, Nature Astronomy (202his article is republished from The Conversation under a Creative Commons license. Read the original article.
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