NEWS & PRESS
42 million light years away, 20 million times the mass of the Sun, and coming back to life. A team of radio astronomers, led by Dr Megan Argo of the Jodrell Bank Centre for Astrophysics, are watching a previously dormant black hole wake up in a dramatic display as material falls on to it for the first time for perhaps millions of years. Dr Argo reported their work today (9 July) at the National Astronomy Meeting at Venue Cymru, in Llandudno, Wales.
NGC 660 is a stunning example of a polar ring system galaxy. Like most galaxies, it has a thick disk of stars and gas. But NGC 660 also hosts a larger and much less dense ring of stars and smaller star-forming clouds, in orbit over its poles. This additional ring is thought to be the remnants of a past encounter with another galaxy that disrupted both systems.
In 2012, astronomers carrying out a survey with the Arecibo radio telescope in Puerto Rico noticed that NGC 660 had suddenly become hundreds of times brighter over just a few months. Normal galaxies do not change their brightness very quickly as they are very large systems made of many (relatively) small individual components in the form of stars, gas and dust. Though all of these may change dramatically, the average brightness of a galaxy tends to be very stable.
The earlier results mean that one particular object within the galaxy has undergone a significant change and become much brighter, and the likely culprit is either an exploding star, or the central supermassive black hole. But the Arecibo observations could only hint at what was happening.
Individual radio dishes have very poor resolution, so astronomers link widely spaced telescopes together to simulate a much larger instrument – a technique known as interferometry. With the various networks of telescopes working in this way, the team could then look at NGC 660 in detail.
The new images show features about a light year across, about a quarter of the distance between the Sun and Alpha Centauri, the next nearest star. They reveal a new, very bright radio source in the very centre of NGC 660, right where we expect to find the central supermassive black hole.
Inactive black holes do not emit large amounts of radiation, so we can only detect them by their gravitational effect on the orbits of stars around them. But the black hole in NGC 660 is now very obvious, and is many hundreds of times brighter than anything seen in the centre of NGC 660 in the archive of radio images before 2010.
Dr Argo said: “Many examples of galaxies with active black holes are already known, often with massive jets stretching millions of light years into intergalactic space. But NGC 660 is special – for the first time we can see this activity starting up.”
The Westerbork observations let the team use this new strong radio source to probe the normally opaque clouds of hydrogen gas within the galaxy, shining a ‘torch’ through the clouds to see what they are made of. The parallel results from e-MERLIN show that the object is slowly fading, and is similar to other galaxies with more mature systems, and the highest resolution images from the EVN show evidence of a high-speed jet of material leaving the vicinity of the black hole.
Material (gas, dust and stars) near a black hole can sit in stable orbits around the central massive object for a long time, but eventually it loses energy, spirals in, and falls onto the black hole. At the same time, some material is ejected and this seems to have created the outburst and jet now seen in NGC 660.
Material in the jet is very fast, travelling at about 10% of the speed of light. Dr Argo explained: “Nothing on Earth has anything like the energy of a jet leaving a giant black hole. Because it moves so quickly, we should be able to watch the material travelling out over the next few years and measure its speed and energy. The big question is whether it has enough energy to overcome gravity, and punch its way out of the galaxy, or if it will fizzle out before getting that far.”
Studying the jet will give astronomers a clue about the initial eruption of the jet, and how much material fell onto the black hole to cause the outburst in the first place.
Dr Sam Lindsay
Dr Megan Argo
Notes for editors
The Royal Astronomical Society National Astronomy Meeting (NAM 2015) will take place in Venue Cymru, Llandudno, Wales, from 5-9 July. NAM 2015 will be held in conjunction with the annual meetings of the UK Solar Physics (UKSP) and Magnetosphere Ionosphere Solar-Terrestrial physics (MIST) groups. The conference is principally sponsored by the Royal Astronomical Society (RAS) and the Science and Technology Facilities Council (STFC). Follow the conference on Twitter
The Royal Astronomical Society (RAS), founded in 1820, encourages and promotes the study of astronomy, solar-system science, geophysics and closely related branches of science. The RAS organises scientific meetings, publishes international research and review journals, recognizes outstanding achievements by the award of medals and prizes, maintains an extensive library, supports education through grants and outreach activities and represents UK astronomy nationally and internationally. Its more than 3800 members (Fellows), a third based overseas, include scientific researchers in universities, observatories and laboratories as well as historians of astronomy and others. Follow the RAS on Twitter
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