Washington: The International LOFAR Telescope has made the first images of galaxy cluster Abell 2256 in the frequency range of 20 to 60 MHz.
Abell 2256 is a cluster containing hundreds of galaxies at a distance of 800 million light-years.
An international team of astronomers is using the telescope from ASTRON, the Netherlands Institute for Radio Astronomy, to study the formation of the galaxy cluster.
“The structure we see in the radio images made with LOFAR provides us with information about the origin of this cluster,” explained lead author Dr. Reinout van Weeren (Leiden University and ASTRON).
The research involved a large team of scientists from 26 different universities and research institutes.
What came as a surprise to scientists was that the cluster of galaxies was brighter and more complex than expected.
“We think that galaxy clusters form by mergers and collisions of smaller clusters,” said Dr. van Weeren.
Abell 2256 is a prime example of a cluster that is currently undergoing a collision. The radio emission is produced by tiny elementary particles that move nearly at the speed of light.
With LOFAR it is possible to study how these particles get accelerated to such speeds.
“In particular, we will learn how this acceleration takes place in regions measuring more than 10 million light-years across,” said Dr. Gianfranco Brunetti from IRA-INAF in Bologna, Italy, who together with Prof. Marcus Brüggen from the Jacobs University in Bremen, coordinates the LOFAR work on galaxy clusters.
LOFAR was built by a large international consortium led by the Netherlands and which includes Germany, France, the United Kingdom and Sweden.
One of the main goals of LOFAR is to survey the entire northern sky at low radio frequencies, with a sensitivity and resolution about 100 times better than what has been previously done. Scientists believe that this survey will discover more than 100 million objects in the distant universe.
“Soon we will start our systematic surveys of the sky that will lead to great discoveries,” stated Prof. Huub Rolttgering from Leiden University and Principal Investigator of the LOFAR Survey Key Project.
The study will be published in the scientific journal Astronomy & Astrophysics.