The discovery set in motion the hunt for more of these ‘changing-look’ quasars. The search has identified dozens of these mysterious beasts, some of which have dimmed more dramatically than the first. The two studies published this month on the preprint server arXiv suggest that these quasars blaze out of existence because the amount of gas and dust flowing through their accretion disks — the swirl of hot matter that encircles a black hole — drops dramatically. In effect, the black hole starves.
In one study, Zhenfeng Sheng, an astronomer at the University of Sciences and Technology of China in Hefei, and his colleagues peered closely at ten changing-look quasars that had been previously imaged by the Sloan Digital Sky Survey and NASA’s Wide-Field Infrared Survey Explorer1. By looking at these quasars in both optical and infrared wavelengths, the team could probe both the quasar’s accretion disk and its torus — the doughnut-shaped ring of dust clouds that wraps around it.
This approach worked because the glowing accretion disk sends optical light towards the dark torus, where it is absorbed and re-emitted as infrared light. Any change to the torus’s light mirrors a change to the accretion disk’s light. So when Sheng and his colleagues found that the optical light emitted by each quasar dimmed before the infrared light did, they knew it was caused by a drop in the amount of material flowing through the accretion disk.
The other study, led by astronomer Damien Hutsemékers of the University of Liège in Belgium, reinforces this idea. Hutsemékers’ team examined the light emanating from a single changing-look quasar. Some of this light is polarized as it passes through regions around the quasar that are thought to be rich in electrons, just as molecules in Earth's atmosphere scatter and polarize light from the Sun.
The researchers were trying to determine whether a dust cloud was blocking the quasar’s accretion disk; if it was, more of the light from the quasar would appear to come from the polarizing regions. But the team did not detect an increase in polarized light from the quasar once it started dimming. This rules out the presence of a dust cloud, but not changes in the accretion disk.
Nicholas Ross, an astronomer at the University of Edinburgh, UK, says that the two studies’ results are intriguing, if preliminary.
A peek at primordial galaxies
If astronomers can pin down the mechanism behind changing-look quasars, and the timescales on which these objects wink out of existence, it could help them to better understand how galaxies evolve.
Every massive galaxy is thought to have hosted a quasar in its early years. The supermassive black holes in quasars can release winds strong enough to halt star formation in a young galaxy. Over time, a galaxy that hosted a stable quasar for long periods may look very different to one with a quasar that behaved unpredictably. One way to think about it is to picture two identical bathtubs full of water, says Meg Urry, an astronomer at Yale University in New Haven, Connecticut. Pouring a cup of boiling water into one and a couple of litres of lukewarm water into the other would give bathers very different experiences, she notes.
Uncovering the inner workings of changing-look quasars could also help astronomers to trace how gas and dust flows into a black hole. Although the latest results suggest that changing-look quasars dim dramatically because they run out of fuel, researchers still can’t explain how that would happen in such a short time.
But LaMassa, who was one of the chairs of the first conference on changing-look quasars in July along with Ross, thinks that the field is on the right track. “There are a lot of questions still to be answered,” she says. “But I think we’re asking the right questions and going in the right direction.”