Numerical simulations of the mass density of the gas orbiting the black hole on equatorial slices shortly after merger. Selected for an Editors’ Suggestion.

From the article:

Merger of Spinning, Accreting Supermassive Black Hole Binaries
Lorenzo Ennoggi, Manuela Campanelli, Julian Krolik, Scott C. Noble, Yosef Zlochower, and Maria Chiara de Simone
Phys. Rev. Lett. 136, 111401 (2026)

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