
Credit: Cardiff University
Astronomers zoom in on black hole with one of the lowest masses ever observed in nearby "ghost" galaxy.
"On the left is shown a color composite Hubble Space Telescope image of the centre of `Mirachs Ghost'. On the right is shown the new ALMA image of this same region, revealing the distribution of the cold, dense gas that swirls around this centre of this object in exquisite detail."
A research team led by Cardiff University scientists say they are closer to understanding how a supermassive black hole (SMBH) is born thanks to a new technique that has enabled them to zoom in on one of these enigmatic cosmic objects in unprecedented detail.
Scientists are unsure as to whether SMBHs were formed in the extreme conditions shortly after the big bang, in a process dubbed a 'direct collapse', or were grown much later from 'seed' black holes resulting from the death of massive stars.
If the former method were true, SMBHs would be born with extremely large masses - hundreds of thousands to millions of times more massive than our Sun - and would have a fixed minimum size.
If the latter were true then SMBHs would start out relatively small, around 100 times the mass of our Sun, and start to grow larger over time by feeding on the stars and gas clouds that live around them.
Astronomers have...