A team of astrophysicists has discovered that supermassive black holes at the centre of galaxies aren't just destroyers of stars, but can also be their creators.

Stellar black holes form from the collapse of a large star. They can have a mass of 20 times that of of our sun or higher, and they consume anything that gets too close, including a star.

There's another category of these stellar gourmands: supermassive black holes. These have masses more than one billion times that of the sun and lurk at the centre of most galaxies, including our own.

While it was suspected that these supermassive black holes could actually be giving rise to new stars while simultaneously destroying unfortunate interlopers, there wasn't enough direct evidence to support that theory. Until now.

Recently, a team of European astronomers was observing the collision of two galaxies some 600 million light-years away — each with a supermassive black hole at its centre — using the Very Large Telescope (VLT) in Chile. There, they found evidence of new star birth from material being ejected from the black hole, called an outflow.

While it might seem a contradiction that nothing can escape a black hole, but an outflow of gas is responsible for creating new stars, it's all about the location: nothing can escape a black hole once it gets so close that all matter is sucked in and can't escape.

However, the gases that swirl around the centre of the black hole — think of water going down a drain — exist in something called an accretion disc.

It's from there that gases are heated to incredible temperatures and then are rapidly ejected into space. Astronomers believe that some of the material might be flung out of the galaxy altogether.

This illustration shows a doomed star (orange circle) that wanders so close to a giant black hole that the enormous gravity stretches the star until it is torn apart. Some of the star's mass (white stream) is swallowed by the black hole, while the rest is flung away into the surrounding galaxy. (M.Weiss/NASA/CXC)

The stars that have been created lie a good distance from the supermassive black hole, some about 100 light-years away, while others considerably farther, perhaps 5,000 to 10,000 light years away,

Some of these stars might eventually fall back into the supermassive black hole in a type of recycling, while others may end up on the far edges of the galaxy's spiral arms, or even out of it.

The newly discovered stars are much larger than our own sun: about 10 times its mass, said Roberto Maiolino, an astrophysicist and lead author of the paper that was published Monday in the journal Nature.

They could even be 40 or 50 times as large as our sun. In terms of a universal time scale, they are considered infants, believed to be less than a few tens of millions years old.

Changing the theories

The discovery is exciting for astronomers and could reshape the theory on galactic formation.

While spiral galaxies have a bulge of stars at their centre and a diffuse cloud of stars called a halo, elliptical galaxies are mostly spheroidal. If stars are formed by this type of outflow, however, it could explain the shape of galaxies.

"If this is common, as some models predicted ... this could change quite drastically our understanding of galaxy formation evolution," Maiolino told CBC News. "It is a completely new mode of forming stars in galaxies."

As well, this could help explain how heavy elements have come to exist in the space between galaxies, called the interstellar medium.

Maiolino said the team has begun searching more galactic cores for more cases of this type of stellar formation.

"The next step is to understand whether this is a peculiar system in which this phenomenon is taking place or it is common," he said.

Though studying galactic cores is a difficult task, he said he hopes that, with the launch of the James Webb Space Telescope in 2018, more research can be done.