We commonly think of black holes as cosmic destroyer , heartlessly devouring anything — even a star — that get in their enormous gravitative twist . But there might be another , more helpful side to supermassive smuggled holes that we ’re only just discovering .

A team of researchers in Australia and the United Kingdom say they ’ve let on something very strange in the nearby Galax urceolata Centaurus A : its key , supermassive contraband hole in reality seems to be helping fresh star topology to form . We know that bleak holes can become “ switch on ” , supercharging the stuff around it and push it away , which creates a phenomenon know as an “ leakage . ” These outflows demolish through star - forming gas notice elsewhere in the Galax urceolata , heating and compressing the gas as it passes by .

In a statement , the Royal Astronomical Society explains how the astronomers used information — some of which you may see in the picture up top — from the Hubble telescope ’s Wide Field Camera 3 to learn the outcome of these outflows :

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With WFC3 , the scientists convey a close look at the ‘ inner filament ’ , a neighborhood locate nigh to the outflow that is a source of ultraviolet and X - ray emission , as well as being bright in seeable light . Using the Hubble images , the squad were then capable to map out the star formation history of the strand with unprecedented truth .

They find that the tip of the filum penny-pinching to the outflow contains young superstar , the ages of which are similar to the time since the outflow ‘ switched on ’ but that there are no young stars further up the filum . This is exactly what is expected from an outflow overrun a cloud of flatulence sitting in its way . The densest fundamental parts of the swarm are pack together and founder to form star , while the flatulence on the outskirts is sweep forth from the tip of the filament , like a pile of autumn leaves in the wind .

Without the smuggled hole ’s leak , the gaseous state might never have become tightly compressed enough to start the formation of new stars . Team loss leader Dr. Stanislav Shabala of the University of Tasmania says that these bootleg hole outflows would have been especially important in the early population , when galaxies were full of dense pocket of gas just waiting to start flux into stars .

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ViaMonthly Notices of the Royal Astronomical Society . Image of the inner filum by Mark Crockett .

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