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| Fältnamn | Indikatorer | Metadata |
|---|---|---|
| 000 | 06867naa a2201477 4500 | |
| 001 | oai:research.chalmers.se:7e16bb35-b32c-43db-a46c-a0fa3d55c265 | |
| 003 | SwePub | |
| 008 | 171007s2012 | |||||||||||000 ||eng| | |
| 024 | 7 | a https://doi.org/10.1051/0004-6361/2012191542 DOI |
| 024 | 7 | a https://research.chalmers.se/publication/1632892 URI |
| 040 | a (SwePub)cth | |
| 041 | a engb eng | |
| 042 | 9 SwePub | |
| 072 | 7 | a art2 swepub-publicationtype |
| 072 | 7 | a ref2 swepub-contenttype |
| 100 | 1 | a van Weeren, R. J.4 aut |
| 245 | 1 0 | a First LOFAR observations at very low frequencies of cluster-scale non-thermal emission: the case of Abell 2256 |
| 264 | c 2012-06-25 | |
| 264 | 1 | b EDP Sciences,c 2012 |
| 338 | a electronic2 rdacarrier | |
| 520 | a Abell 2256 is one of the best known examples of a galaxy cluster hosting large-scale diffuse radio emission that is unrelated to individual galaxies. It contains both a giant radio halo and a relic, as well as a number of head-tail sources and smaller diffuse steep-spectrum radio sources. The origin of radio halos and relics is still being debated, but over the last years it has become clear that the presence of these radio sources is closely related to galaxy cluster merger events. Here we present the results from the first LOFAR low band antenna (LBA) observations of Abell 2256 between 18 and 67 MHz. To our knowledge, the image presented in this paper at 63 MHz is the deepest ever obtained at frequencies below 100 MHz in general. Both the radio halo and the giant relic are detected in the image at 63 MHz, and the diffuse radio emission remains visible at frequencies as low as 20 MHz. The observations confirm the presence of a previously claimed ultra-steep spectrum source to the west of the cluster center with a spectral index of -2.3 +/- 0.4 between 63 and 153 MHz. The steep spectrum suggests that this source is an old part of a head-tail radio source in the cluster. For the radio relic we find an integrated spectral index of -0.81 +/- 0.03, after removing the flux contribution from the other sources. This is relatively flat which could indicate that the efficiency of particle acceleration at the shock substantially changed in the last similar to 0.1 Gyr due to an increase of the shock Mach number. In an alternative scenario, particles are re-accelerated by some mechanism in the downstream region of the shock, resulting in the relatively flat integrated radio spectrum. In the radio halo region we find indications of low-frequency spectral steepening which may suggest that relativistic particles are accelerated in a rather inhomogeneous turbulent region. | |
| 650 | 7 | a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe |
| 650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng |
| 653 | a galaxies: clusters: individual: Abell | |
| 653 | a deep | |
| 653 | a astrophysical shocks | |
| 653 | a coma cluster | |
| 653 | a shock acceleration | |
| 653 | a sky survey | |
| 653 | a x-ray-emission | |
| 653 | a radio continuum: general | |
| 653 | a 1.4 ghz | |
| 653 | a particle-acceleration | |
| 653 | a magnetic-fields | |
| 653 | a telescopes | |
| 653 | a extended radio-emission | |
| 653 | a merging galaxy cluster | |
| 700 | 1 | a Rottgering, H.4 aut |
| 700 | 1 | a Rafferty, D.4 aut |
| 700 | 1 | a Pizzo, R.4 aut |
| 700 | 1 | a Bonafede, A.4 aut |
| 700 | 1 | a Brüggen, M.4 aut |
| 700 | 1 | a Brunetti, G.4 aut |
| 700 | 1 | a Ferrari, C.4 aut |
| 700 | 1 | a Orru, E.4 aut |
| 700 | 1 | a Heald, G.4 aut |
| 700 | 1 | a McKean, J. P.4 aut |
| 700 | 1 | a Tasse, C.4 aut |
| 700 | 1 | a De Gasperin, F.4 aut |
| 700 | 1 | a Birzan, L.4 aut |
| 700 | 1 | a van Zwieten, J. E.4 aut |
| 700 | 1 | a van der Tol, S.4 aut |
| 700 | 1 | a Shulevski, A.4 aut |
| 700 | 1 | a Jackson, N.4 aut |
| 700 | 1 | a Offringa, A. R.4 aut |
| 700 | 1 | a Conway, John,d 1963u Chalmers tekniska högskola,Chalmers University of Technology4 aut0 (Swepub:cth)jconway |
| 700 | 1 | a Intema, H. T.4 aut |
| 700 | 1 | a Clarke, T. E.4 aut |
| 700 | 1 | a van Bemmel, I.4 aut |
| 700 | 1 | a Miley, G. K.4 aut |
| 700 | 1 | a White, G. J.4 aut |
| 700 | 1 | a Hoeft, M.4 aut |
| 700 | 1 | a Cassano, R.4 aut |
| 700 | 1 | a Macario, G.4 aut |
| 700 | 1 | a Morganti, R.4 aut |
| 700 | 1 | a Wise, M. W.4 aut |
| 700 | 1 | a Horellou, Cathy,d 1967u Chalmers tekniska högskola,Chalmers University of Technology4 aut0 (Swepub:cth)horellou |
| 700 | 1 | a Valentijn, E. A.4 aut |
| 700 | 1 | a Wucknitz, O.4 aut |
| 700 | 1 | a Kuijken, K.4 aut |
| 700 | 1 | a Ensslin, T. A.4 aut |
| 700 | 1 | a Anderson, J.4 aut |
| 700 | 1 | a Asgekar, A.4 aut |
| 700 | 1 | a Avruch, I. M.4 aut |
| 700 | 1 | a Beck, R.4 aut |
| 700 | 1 | a Bell, M. E.4 aut |
| 700 | 1 | a Bell, M. R.4 aut |
| 700 | 1 | a Bentum, M. J.4 aut |
| 700 | 1 | a Bernardi, G.4 aut |
| 700 | 1 | a Best, P.4 aut |
| 700 | 1 | a Boonstra, A. J.4 aut |
| 700 | 1 | a Brentjens, M.4 aut |
| 700 | 1 | a van de Brink, R. H.4 aut |
| 700 | 1 | a Broderick, J.4 aut |
| 700 | 1 | a Brouw, W. N.4 aut |
| 700 | 1 | a Butcher, H. R.4 aut |
| 700 | 1 | a van Cappellen, W.4 aut |
| 700 | 1 | a Ciardi, B.4 aut |
| 700 | 1 | a Eisloffel, J.4 aut |
| 700 | 1 | a Falcke, H.4 aut |
| 700 | 1 | a Fender, R.4 aut |
| 700 | 1 | a Garrett, M. A.4 aut |
| 700 | 1 | a Gerbers, M.4 aut |
| 700 | 1 | a Gunst, A.4 aut |
| 700 | 1 | a van Haarlem, M. P.4 aut |
| 700 | 1 | a Hamaker, J. P.4 aut |
| 700 | 1 | a Hassall, T.4 aut |
| 700 | 1 | a Hessels, J. W. T.4 aut |
| 700 | 1 | a Koopmans, L. V. E.4 aut |
| 700 | 1 | a Kuper, G.4 aut |
| 700 | 1 | a van Leeuwen, J.4 aut |
| 700 | 1 | a Maat, P.4 aut |
| 700 | 1 | a Millenaar, R.4 aut |
| 700 | 1 | a Munk, H.4 aut |
| 700 | 1 | a Nijboer, R.4 aut |
| 700 | 1 | a Noordam, J. E.4 aut |
| 700 | 1 | a Pandey, V. N.4 aut |
| 700 | 1 | a Pandey-Pommier, M.4 aut |
| 700 | 1 | a Polatidis, A.4 aut |
| 700 | 1 | a Reich, W.4 aut |
| 700 | 1 | a Scaife, A. M. M.4 aut |
| 700 | 1 | a Schoenmakers, A.4 aut |
| 700 | 1 | a Sluman, J.4 aut |
| 700 | 1 | a Stappers, B. W.4 aut |
| 700 | 1 | a Steinmetz, M.4 aut |
| 700 | 1 | a Swinbank, J.4 aut |
| 700 | 1 | a Tagger, M.4 aut |
| 700 | 1 | a Tang, Y.4 aut |
| 700 | 1 | a Vermeulen, R.4 aut |
| 700 | 1 | a de Vos, M.4 aut |
| 710 | 2 | a Chalmers tekniska högskola4 org |
| 773 | 0 | t Astronomy and Astrophysicsd : EDP Sciencesg 543, s. Article Number: A43 -q 543<Article Number: A43 -x 0004-6361x 1432-0746 |
| 856 | 4 | u http://publications.lib.chalmers.se/records/fulltext/local_163289.pdfx primaryx freey FULLTEXT |
| 856 | 4 | u https://www.aanda.org/articles/aa/pdf/2012/07/aa19154-12.pdf |
| 856 | 4 8 | u https://doi.org/10.1051/0004-6361/201219154 |
| 856 | 4 8 | u https://research.chalmers.se/publication/163289 |
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- Wise, M. W.
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- Beck, R.
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