Figure 1 Composite image showing how
powerful radio jets from the supermassive black hole at the center of a galaxy in the Phoenix Cluster inflated huge «bubbles» in the hot, ionized gas surrounding the galaxy (the cavities inside the blue region imaged by NASA's Chandra X-ray observatory).
Powerful radio jets from the black hole — which normally suppress star formation — are stimulating the production of cold gas in the galaxy's extended halo of hot gas.
Powerful radio jets from the black hole - which normally suppress star formation - are stimulating the production of cold gas in the galaxy's extended halo of hot gas.
Powerful radio jets from the supermassive black hole at the center of the galaxy are creating giant radio bubbles (blue) in the ionized gas surrounding the galaxy.
Not exact matches
Gullberg and her colleagues believe that the explanation lies with
powerful jets of
radio waves that are ejected from a supermassive black hole at the centre of the Spiderweb Galaxy.
Statistical analysis of supermassive black holes suggests that the spin of the black hole may play a role in the generation of
powerful high - speed
jets blasting
radio waves and other radiation across the Universe.
«Observations with the next generation of
radio telescopes will tell us more about what actually happens when a star is eaten by a black hole — and how powerful jets form and evolve right next to black holes,» explains Stefanie Komossa, astronomer at the Max Planck Institute for Radio Astronomy in Bonn, Ger
radio telescopes will tell us more about what actually happens when a star is eaten by a black hole — and how
powerful jets form and evolve right next to black holes,» explains Stefanie Komossa, astronomer at the Max Planck Institute for
Radio Astronomy in Bonn, Ger
Radio Astronomy in Bonn, Germany.
As a result of this massive «meal» the black hole begins to launch a
powerful jet that we can detect with
radio telescopes.
Radio data shows that the supermassive black hole at the center of NGC 4258 is producing
powerful jets of high - energy particles.