Highlights — Some exciting recent scientific results from our group

Swirling Electrons in the Whirlpool Galaxy
Cosmic particles and magnetic fields in the galaxy M51 observed with the LOFAR radio telescope

The whirlpool galaxy Messier 51 (M51) is seen from a distance of approximately 30 million light years. This galaxy appears almost face-on and displays a beautiful system of spiral arms.
A European team of astronomers was able to observe M51 with the International LOFAR Telescope in the frequency range 115-175 MHz, just above the normal commercial FM radio frequency band of 88-108 MHz. The team obtained the most sensitive image of any galaxy at frequencies below 1 GHz so far. With LOFAR's high sensitivity, the disk of M51 in the radio regime could be traced much further out than before. The astronomers detected cosmic electrons and magnetic fields 40,000 light years away from the center of M51.
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Radio-burst discovery deepens astrophysics mystery
Newly detected short radio pulse appears to come from far beyond our galaxy

The discovery of a split-second burst of radio waves using the Arecibo radio telescope in Puerto Rico provides important new evidence of mysterious pulses that appear to come from deep in outer space. The findings by an international team of astronomers led by Laura Spitler from the Max Planck Institute for Radio Astronomy in Bonn, Germany are published on July 10 in the online issue of The Astrophysical Journal. They mark the first time that a so-called "fast radio burst" has been detected in the Northern hemisphere of the sky.
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Trio of supermassive black holes shake space-time
Tight system of black holes in a distant galaxy

Astronomers have discovered three closely orbiting supermassive black holes in a galaxy more than 4 billion light years away. This is the tightest trio of black holes known to date and is remarkable since most galaxies have just one black hole, usually with a mass between 1 million to 10 billion times that of the Sun, at their centre. The discovery suggests that such closely packed supermassive black holes are far more common than previously thought.
An international research team, including Hans-Rainer Klöckner from the Max Planck Institute for Radio Astronomy in Bonn, Germany, performed VLBI (Very Long Baseline Interferometry) observations with radio telescopes at a number of frequencies to discover the inner two black holes of the triple system. The VLBI technique combines the signals from large radio antennas separated by up to 10. 000 kilometres to see details 50 times finer than that possible with the Hubble Space Telescope. In this project the Effelsberg 100m radio telescope took part in European VLBI network (EVN) observations covering two radio frequencies.
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An Exotic Millisecond Pulsar Trio
Stellar astrophysicists probe new territory with the discovery of a neutron star orbited by two white dwarfs
Millisecond pulsars are old neutron stars, with rotational frequencies of several hundred revolutions per second. Previous theoretical studies have explained their origin via mass transfer in binary systems. However, the first discovery of a millisecond pulsar in a triple system is quite a surprise and challenges current consensus. The astrophysicist Thomas Tauris from the Max Planck Institute for Radio Astronomy and the Argelander Institute for Astronomy in Bonn, has developed a semi-analytical model, jointly with Ed van den Heuvel from the University of Amsterdam, which can resolve the puzzling formation of this exotic triple system. Through theoretical calculations and stability analysis on the base of stellar evolution, they have demonstrated a plausible theoretical model which brings new insight to our knowledge of stellar interactions in multiple star systems. Their study can also help explain an increasing number of observed binary millisecond pulsars which seem to require a triple system origin. more
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