EDP Sciences Journals List
Advanced Search
Free access article

Issue A&A
Volume 423, Number 1, August III 2004
Page(s) 111 - 119
Section Extragalactic astronomy
DOI http://dx.doi.org/10.1051/0004-6361:20040316



A&A 423, 111-119 (2004)
DOI: 10.1051/0004-6361:20040316

Spectral index maps of the radio halos in Abell 665 and Abell 2163

L. Feretti1, E. Orrù1, G. Brunetti1, G. Giovannini1, 2, N. Kassim3 and G. Setti1, 2

1  Istituto di Radioastronomia - CNR, via P. Gobetti 101, 40129 Bologna, Italy
    e-mail: iferetti@ira.cnr.it
2  Dipartimento di Astronomia, Univ. Bologna, via Ranzani 1, 40127 Bologna, Italy
3  Naval Research Laboratory, Code 7213, Washington DC 20375, USA

(Received 23 February 2004 / Accepted 14 April 2004)

Abstract
New radio data at 330 MHz are presented for the rich clusters Abell 665 and Abell 2163, whose radio emission is characterized by the presence of a radio halo. These images allowed us to derive the spectral properties of the two clusters under study. The integrated spectra of these halos between 0.3 GHz and 1.4 GHz are moderately steep: $\alpha^{1.4}_{0.3} = 1.04$ and $\alpha^{1.4}_{0.3} = 1.18$, for A665 and A2163, respectively. The spectral index maps, produced with an angular resolution of the order of ~1´, show features of the spectral index (flattening and patches), which are indication of a complex shape of the radiating electron spectrum, and are therefore in support of electron reacceleration models. Regions of flatter spectrum are found to be related to the recent merger activity in these clusters. This is the first strong confirmation that the cluster merger supplies energy to the radio halo. In the undisturbed cluster regions, the spectrum steepens with the distance from the cluster center. This is interpreted as the result of the combination of the magnetic field profile with the spatial distribution of the reacceleration efficiency, thus allowing us to set constraints on the radial profile of the cluster magnetic field.


Key words: radio continuum: general -- galaxies: clusters: general -- galaxies: clusters: individual: A665 -- galaxies: clusters: individual: A2163 -- galaxies: intergalactic medium -- X-rays: galaxies: clusters

SIMBAD Objects



© ESO 2004


What is OpenURL?

The OpenURL standard is a protocol for transmission of metadata describing the resource that you wish to access. An OpenURL link contains article metadata and directs it to the OpenURL server of your choice. The OpenURL server can provide access to the resource and also offer complementary services (specific search engine, export of references...). The OpenURL link can be generated by different means.
  • If your librarian has set up your subscription with an OpenURL resolver, OpenURL links appear automatically on the abstract pages.
  • You can define your own OpenURL resolver with your EDPS Account. In this case your choice will be given priority over that of your library.
  • You can use an add-on for your browser (Firefox or I.E.) to display OpenURL links on a page (see http://www.openly.com/openurlref/). You should disable this module if you wish to use the OpenURL server that you or your library have defined.