BBC Sky at Night Magazine

Black hole jets could be hiding in plain sight

A new discovery could explain how active and calm galaxies co-habit the same regions

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ou might assume it would be difficult to confuse a galaxy and a star, and yet that’s the story of ‘BL Lac’ objects, the engimas at the heart of this month’s paper. Named after the first example that was found in the otherwise obscure constellat­ion of Lacerta, these objects show rapid and significan­t changes in brightness, and were originally thought to be a rare form of variable star. We now know that their light comes not from a star at all, but from the centres of active galaxies, as material falls onto the supermassi­ve black holes that lurk there.

When enough material falls towards the centre of a galaxy, first an accretion disc forms – as seen in those wonderful images from the Event Horizon Telescope, released last year – and then some can be expelled in a rapidly moving jet. In the case of BL Lac objects, conditions are so extreme that the jets sometimes seem (thanks to a quirk of geometry) to be moving faster than the speed of light.

The strange behaviour of BL Lac might be explained if we’re staring down the barrel of the jet itself. The rapid changes in brightness seen in both visible light and at radio wavelength­s are then explained by the behaviour of material in the jet, rather than around the black hole itself. Testing this idea is hard, though, and the authors of this month’s paper have had a good idea.

Assembling a collection of massive elliptical galaxies which host BL Lac objects, they look at their environmen­ts, and whether they’re found in dense clusters of galaxies, the middle of empty voids, or somewhere in between. This is difficult to do precisely, but a good estimate can be made just by counting a system’s neighbours – after all, if you have more neighbours you live in a more crowded area!

Once the count is complete, comparison­s can be made with other sorts of objects – in this case, with other types of active galaxies. If we get a BL Lac when we stare down the jet, there should be a whole

“BL Lac objects show rapid and significan­t changes in brightness, and were originally thought to be a rare form of variable star”

Ypopulatio­n of galaxies out there which are the same, except that the jet points in another direction. Those other systems should be found in the same kind of environmen­t.

The prime candidate is a type of active galaxy called an FR I, but the authors show convincing­ly that these live in more crowded environmen­ts, and so they can’t be the ‘hidden’ BL Lacs. However, the BL Lacs do match another population in environmen­t: they live in the same places in the Universe as a type of galaxy called an FR 0. These are essentiall­y bright points of radio emission. This result is itself a mystery – why should the most spectacula­r examples of active galaxies share an environmen­t with these relatively quiet systems? One answer, proposed by the team, is that the high energy jets we see in the most active systems are actually a ubiquitous feature of galaxies with growing black holes. If the jet points towards us, we get a BL Lac, and if it doesn’t we see a nice, quiet system. If jets really are this common, we’ll need to explain how such jets form – and can expect a jet to have been a feature of our own Milky Way’s past.

 ??  ?? Do the high energy jets we see in the most active systems, suggest growing black holes?
Chris Lintott
Do the high energy jets we see in the most active systems, suggest growing black holes? Chris Lintott
 ??  ?? Prof Chris Lintott is an astrophysi­cist and co-presenter on The Sky at Night
Prof Chris Lintott is an astrophysi­cist and co-presenter on The Sky at Night

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