... that around 1 - 2 billion years ago, a merger between two galaxies – each with central, massive black holes – took place. As the two black holes did not have the same mass and rotation rate, gravitational waves created as the...
... rest of the galaxy put together. It is believed that this outpouring of radiation is a result of the accretion of matter by a supermassive black hole at the centre of its host galaxy and as the energy is dispersed, it heats and dispels the gas that...
... characteristics at very high precision. STIS was integral to effectively observing the low-luminosity region around the black hole, blocking out the galaxy’s brilliant light. The astronomers initially selected this galaxy to validate accepted models...
... named LB-1 by the researchers. The discovery is reported in the latest issue of Nature. The discovery came as a big surprise. "Black holes of such mass should not even exist in our Galaxy, according to most of the current models of stellar evolution...
...not able to escape from their cores due to the tremendous amount of gravity the black hole creates. Instead the primary method of detecting a black hole is through observations of radio or X-ray emissions coming from hot material around them. However...
...were lucky enough to notice three bright flares from around the black hole — it was a lucky coincidence!" The emission from the ... theoretical predictions for hot spots orbiting close to a black hole with a mass 1.3 trillion times greater than the ...