Astronomers have found evidence of large numbers of black holes in galaxy Arp 220. Jets which give off strong radio waves are created in binary star systems like this one. Gas is drawn in from a red supergiant star (left) and collects in a bright disc of hot gas which slowly feeds an (unseen) black hole in its centre, from which the jets are shot out into space.
Image: Artist’s impression: ESO/L. Calçada/M.Kornmesser)
A team led by astronomers at Chalmers University of Technology and Onsala Space Observatory has been monitoring radio signals from the core of the galaxy Arp 220, which lies 250 million light years from Earth. Besides a number of supernovae, they also found some sources that were at first sight difficult to understand.
“We found three remarkable sources whose brightness was different each time we looked at them. In the beginning we had no idea what they could be” says Fabien Batejat, astronomer at Chalmers, who led the study.
The scientists followed the three peculiar radio sources over several years. Now they think they know what is behind the radio signals: jets created by black holes.
“We believe we are seeing radio emission from binary star systems in which one star has already exploded and left behind a black hole. The black hole “eats” gas which it draws from its companion, producing powerful jets that emit radio waves”, says Fabien Batejat.
The newly discovered black holes in galaxy Arp 220 are only three of many more, the scientists believe.
John Conway, professor of observational radio astronomy at Chalmers and deputy director of Onsala Space Observatory, explains.
“Jets from black holes are visible at this distance only if they are pointing right towards us. Probably there are many more systems like this in this galaxy, but their jets point in other directions”, he says.
The galaxy Arp 220
is already famous for creating new stars at a furious pace. Previous research by the same team has also demonstrated that there are many supernova explosions in the galaxy, up to 250 times more than in our galaxy. Supernovae and black holes are related. Astronomers believe that black holes are created when stars with masses more than about 20 times the sun explode.
In the centre of Arp 220, a galaxy 250 million light years away, scientists at Chalmers have discovered evidence for a large number of black holes.
Image: NASA / ESA / R. Thompson, M. Rieke, G. Schneider (U. of Arizona), N. Scoville (CalTech), A. Evans (U. of Virginia)
This discovery in Arp 220 gives astronomers hope to soon be able to put this idea to the test. Only a dozen black holes of this type are known in the Milky Way, and only a few are known in other galaxies.
“By studying large numbers of these small, star-snacking black holes, we have a new way to learn about how they are created. So far, black hole statistics has only been possible for distant, supermassive black holes”, says Anthony Rushton, member of the team in Onsala.
The discovery was made with a network of radio telescopes around the world, linked together to create very sharp images, using the technique VLBI (Very Long Baseline Interferometry). Radio telescopes can follow events in the dense centers of galaxies that lie behind thick layers of dust, invisible to other telescopes. In order to discover what the radio sources in Arp 220 are, the team made measurements at different radio wavelengths over a period of 17 years.
“This result has only emerged after many years of painstaking observations and improvements in VLBI techniques”, says Philip Diamond, member of the team and Chief of CSIRO Astronomy and Space Science in Australia.
These objects, known to astronomers as microblazars, were theoretically predicted over a decade ago. Astronomers believe microblazars are scaled-down versions of the cosmic beacons known as blazars. In a blazar, a supermassive black hole feasting on dense gas at the centre of a galaxy creates powerful jets which can be observed from Earth if they are directed towards us.
“Our new results from Arp 220 are the best evidence yet for microblazars. It also seems that galaxies like this one can contain very large numbers of them“, says Fabien Batejat.
Previous press release: Astronomers reveal supernova factory:
About the telescopes
The observations were carried out using telescopes which belong to the European VLBI Network (EVN)
together with the Very Long Baseline Array (VLBA).
The VLBA is a set of ten radio telescopes located from Hawaii to St. Croix in the U.S. Virgin Islands and operated by the National Radio Astronomy Observatory.
The EVN is supported by the Joint Institute for VLBI in Europe (JIVE)
About Onsala Space Observatory
Onsala Space Observatory is Sweden's national facility for radio astronomy. The observatory provides researchers with equipment for the study of the earth and the rest of the universe. In Onsala, 45 km south of Gothenburg, it operates two radio telescopes and a station in the international telescope Lofar. It also participates in several international projects. The observatory is hosted by Department of Earth and Space Sciences at Chalmers University of Technology, and is operated on behalf of the Swedish Research Council.
About the team
The team is composed of Fabien Batejat (Onsala Space Observatory, Chalmers University of Technology, Sweden), John Conway (Onsala Space Observatory, Chalmers University of Technology, Sweden), A. Rushton (Onsala Space Observatory; European Southern Observatory, ESO), Rodrigo Parra (ESO, Santiago, Chile), Philip Diamond (CSIRO Astronomy and Space Science, Sydney, Australia); Colin J. Lonsdale (MIT Haystack Observatory, USA) och Carol J. Lonsdale (North American ALMA Science Center, NRAO, Charlottesville, USA).
Robert Cumming, astronomer and communications officer, Onsala Space Observatory, +46-31-772 55 00 or +46-70-493 31 14, email@example.com
Fabien Batejat, astronomer, Onsala Space Observatory, Chalmers University of Technology, +46-31-772 55 00 or +46-76-583 89 96, firstname.lastname@example.org