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A ring-like accretion structure in M87 connecting its black hole and jet - Nature

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A ring-like accretion structure in M87 connecting its black hole and jet - Nature

The nearby radio galaxy M87 is a prime target for studying black hole accretion and jet formation1,2. Event Horizon Telescope observations of M87 in 2017, at a wavelength of 1.3 mm, revealed a ring-like structure, which was interpreted as gravitationally lensed emission around a central black hole3. Here we report images of M87 obtained in 2018, at a wavelength of 3.5 mm, showing that the compact radio core is spatially resolved.

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A ring-like accretion structure in M87 connecting its black hole and jet - Nature

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A ring-like accretion structure in M87 connecting its black hole and jet - Nature

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