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What can we learn from the first M87 Event Horizon Telescope results?

Title:First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole. Abstract: When surrounded by a transparent emission region, black holes are expected to reveal a dark shadow caused by gravitational light bending and photon capture at the event horizon.

What is the minimum wavelength required to resolve the shadows of M87?

VLBI at an observing wavelength of 1.3mm (230GHz) with Earth-diameter-scale baselines is required to resolve the shadows of thecoreofM87(M87* hereafter) and of the Galactic center of Sagittarius A* (SgrA*, Balick & Brown 1974), the two super- massive black holes with the largest apparent angular sizes (Johannsen et al.


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