Dec. 12, 2012 The discovery of a binging black hole in our nearest neighbouring galaxy, Andromeda, has shed new light on some of the brightest X-ray sources seen in other galaxies, according to new work co-authored by astronomers from the International Centre for Radio Astronomy Research's Curtin University node.
Using a suite of Earth-orbiting X-ray telescopes, including NASA's Swift and the European Space Agency's XMM-Newton satellites, a large international team of astronomers watched as the X-ray emission from the black hole -- found over 2million light years away -- brightened and faded over the course of six months.
The study, published in the scientific journal Nature, also shows what happens when black holes feast rapidly on the material stripped from a companion star.
It is the second Ultraluminous X-Ray source (ULX) to have been spotted in Andromeda -- the Milky Way's nearest neighboring galaxy -- in the past two years.
X-ray telescopes have shown many nearby galaxies to host ULX sources, which can be bright enough to outshine an entire galaxy in X-rays.
Astronomers have spent years debating whether these are black holes just a few times the mass of the Sun which are gorging themselves on gas from an orbiting star, or whether they are more massive black holes eating more sedately.
Lead author Dr Matthew Middleton, who led the latest research while at Durham University, said the findings helped solve this debate.
Dr Middleton, now based at the University of Amsterdam, said: "The black hole we observed in Andromeda is the missing link.
"Our observations tell us that this ultraluminous X-ray source -- and by extension, many others -- is just a run-of-the-mill black hole, only about ten times the mass of the Sun, that is swallowing material as fast as it can."
Dr Middleton added: "We watched a black hole go from nibbling daintily at an appetiser to binging on the main course, and then gradually slowing down over dessert."
Black holes in our own Milky Way galaxy are very rarely seen to binge, but when they do, they also launch very powerful beams of material called jets, which are blasted outwards at close to the speed of light, and can be tracked using sensitive radio telescopes.
The team trained the National Science Foundation's Karl G. Jansky Very Large Array on the black hole, and saw extremely bright radio emission that dropped by a half in just 30 minutes.
"Discovering these radio waves from an ultraluminous X-ray source is the smoking gun, a dead giveaway that these are just normal, everyday black holes," said co-author Dr James Miller-Jones, of the Curtin University node of the International Centre for Radio Astronomy Research in Perth, Australia.
"This tells us that the region producing radio waves is extremely small in size, no further across than the distance between Jupiter and the Sun."
This finding was confirmed by zooming in using the world's most eagle-eyed radio telescope, the Very Long Baseline Array.
This was the first time that radio jets had been detected from a stellar-mass black hole outside our own Milky Way galaxy.
Despite the large distance to Andromeda, the absence of dust and gas in that direction allows an unhindered view of the feast, giving scientists key new insights into how jets are produced by a binging black hole.
Co-author Dr Natasha Hurley-Walker, also from the Curtin University node of the International Centre for Radio Astronomy Research, said: "We were very lucky that this ULX appeared in our local neighbourhood; its proximity meant that we could make these radio observations and demonstrate that the black hole emitting the X-rays is fairly small."
ICRAR is a joint venture between Curtin University and The University of Western Australia providing research excellence in the field of radio astronomy.
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The above story is based on materials provided by International Centre for Radio Astronomy Research (ICRAR).
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- Matthew J. Middleton, James C. A. Miller-Jones, Sera Markoff, Rob Fender, Martin Henze, Natasha Hurley-Walker, Anna M. M. Scaife, Timothy P. Roberts, Dominic Walton, John Carpenter, Jean-Pierre Macquart, Geoffrey C. Bower, Mark Gurwell, Wolfgang Pietsch, Frank Haberl, Jonathan Harris, Michael Daniel, Junayd Miah, Chris Done, John S. Morgan, Hugh Dickinson, Phil Charles, Vadim Burwitz, Massimo Della Valle, Michael Freyberg, Jochen Greiner, Margarita Hernanz, Dieter H. Hartmann, Despina Hatzidimitriou, Arno Riffeser, Gloria Sala, Stella Seitz, Pablo Reig, Arne Rau, Marina Orio, David Titterington, Keith Grainge. Bright radio emission from an ultraluminous stellar-mass microquasar in M 31. Nature, 2012; DOI: 10.1038/nature11697
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