The putative center in NGC 1052

We combined observations from three different arrays of radio interferometers: the Event Horizon Telescope (EHT), the Global mm VLBI array (GMVA), and the Very Long Baseline Array (VLBA) to catch the emission from the innermost center in the active galaxy NGC 1052. This is the region where a double sided jet is forming and accelerating up to velocities of half the light speed. To learn more about our most recent results check out our press release: Event Horizon Telescope moving towards a close up of a black hole and its jets.