The formation of these monsters is still not well understood. Nothing can escape because they pretty much suck in everything in the neighborhood. We know that supermassive black holes in the cores of galaxies are tremendously strong gravitational wells. To understand the structures in the latest image, we need to know more about them. Getting the big picture of the black hole

It contains superheated (ionized) matter flowing out at high speed along an axis of rotation. The material streaming away from M87 is an astrophysical jet. 'At this wavelength, we can see how the jet emerges from the ring of emission around the central supermassive black hole,' says Thomas Krichbaum of the Max Planck Institute for Radio Astronomy. The observations, taken in 2018, show the region in radio light emitted at a longer wavelength than the EHT image. It's the first time all three major parts of the object are in the same image. Their combined observations showed very small details in the region around the galactic core. They comprised the Global mm Very Large Baseline Array (GMVA), the Atacama Large Millimeter Array (ALMA), and the Greenland Telescope (GLT). This latest image was made using an extensive array of radio telescopes. It clearly shows the connection between the supermassive black hole, its light ring, and the famous high-speed jet.

This week, they released another amazing view of this monster, this time, in a slightly different range of radio emissions. Now, a team of astronomers from Europe, Korea, and China, have taken things a step further.

Under a falling star by jae