A New View of Galaxy M82

©LOFAR

Galaxy M82

An international team of astronomers led from Chalmers has used the giant radio telescope LOFAR to create the sharpest astronomical image ever taken at very long radio wavelengths.

Made by observing simultaneously from four countries, including Sweden, the image shows the glowing center of the galaxy Messier 82 -- and many bright remnants of supernova explosions.

Astronomers have taken the sharpest image yet of the sky at very long radio wavelengths. The image shows the center of the galaxy Messier 82 (M82), also known as the Cigar Galaxy, 11.5 million light-years from Earth. M82 is forming stars much faster than our galaxy, the Milky Way, and is a favorite object for many astronomers who investigate the evolution of stars and galaxies.

In images taken in visible light, M82 is a riot of stars, gas and dust. LOFAR shows us a completely different scene. In LOFAR's new extremely sharp image we're seeing a collection of bright spots, which are most likely supernova remnants, explains Eskil Varenius (Chalmers), who led the international team of scientists behind the new image. A supernova remnant is a shining shell of shock waves from an exploded star, plowing into its surroundings. Supernova remnants are huge objects by everyday standards, much larger than the size of our own solar system, but look small from a distance.

This galaxy is millions of light-years away, and each remnant can be as little as a few light-years across. We need extremely sharp images to study them, says Eskil Varenius.

The supernova remnants are embedded inside a huge, diffuse cloud of charged particles, or plasma, which absorbs radio waves from these sources. By investigating how different wavelengths pass through the plasma, scientists can learn more about how a gigantic star factory like M82 works.

We're surprised that LOFAR can see as many as 16 bright supernova remnants in M82. This image can give us new clues to the structure of M82 and why so many stars are being formed there, says John Conway, part of the team and director of Onsala Space Observatory where Sweden's LOFAR station is located.

This exciting image of M82 is the first of many that LOFAR and its international stations will be able to give us. The scientists are now working on new super-sharp LOFAR images of other galaxies.

LOFAR is showing us the sky in a way that we've never seen before, and in in exquisite detail. This beautiful image is just a foretaste of what the telescope is capable of, says Mike Garrett, director of ASTRON, the Netherlands Institute for Radio Astronomy.


Reference: "Subarcsecond international LOFAR radio images of the M82 nucleus at 118 MHz and 154 MHz," E. Varenius et al., to be published in Astronomy & Astrophysics (http://www.aanda.org) [preprint: http://arxiv.org/abs/1411.7680].

The team is comprised of Eskil Varenius (Chalmers), John E. Conway (Onsala Space Observatory, Chalmers), Ivan Martí-Vidal (Onsala Space Observatory, Chalmers), R. Beswick (University of Manchester, United Kingdom), A. T. Deller (ASTRON, Netherlands), O. Wucknitz (Max-Planck-Institut für Radioastronomie [MPIfR], Germany), N. Jackson (Manchester), B. Adebahr (MPIfR), M. A. Pérez-Torres (Instituto de Astrofísica de Andalucía, Spain), K. T. Chyzy (Jagiellonian University, Krakow, Poland), Tobia D. Carozzi (Onsala Space Observatory, Chalmers), J. Moldón (ASTRON), Susanne Aalto (Chalmers), R. Beck (MPIfR), P. Best (Royal Observatory Edinburgh, United Kingdom), R.-J. Dettmar (Ruhr-Universität Bochum, Germany), W. van Driel (Observatoire de Paris, France), G. Brunetti (INAF-Istituto di Radioastronomia, Bologna, Italy), M. Brüggen (University of Hamburg, Germany), M. Haverkorn (Radboud University and Leiden University, Netherlands), G. Heald (ASTRON/KAI), Cathy Horellou (Chalmers), M. J. Jarvis (University of Oxford, United Kingdom), L. K. Morabito (Leiden University), G. K. Miley (Leiden University, Netherlands), H. J. A. Röttgering (Leiden University), M. C. Toribio (Astron) and G. J. White (Open University and RAL, UK).

LOFAR (Low Frequency Array) is a radio telescope which consists of thousands of antennas spread across northern Europe with its core in the Netherlands. The telescope is uniquely sensitive to the very longest radio waves that can penetrate Earth's atmosphere. LOFAR is designed and built by ASTRON, the Netherlands Institute for Radio Astronomy. The International LOFAR Telescope has 38 stations in the Netherlands, six in Germany, and one each in France, Sweden and the United Kingdom. Three further stations are under construction in Poland. LOFAR is also a recognized science and technology pathfinder facility for the next-generation radio telescope, the Square Kilometre Array (SKA). Onsala Space Observatory represents Sweden, one of 11 member countries in the SKA Organisation.

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