The large-scale structure of the diffuse radio halo of the Coma cluster at 1.4 GHz

Abstract

We present new measurements of the diffuse radio emission from the Coma cluster of galaxies at 1.4 GHz using the Effelsberg 100-m-telescope. The halo source Coma C has an extent down to noise of about 80 arcmin corresponding to 3 Mpc (H_0 = 50 km/s/Mpc) in Coma. The radio map reveals clear similarities with images of the extended X-ray halo of the Coma cluster. After subtracting the contributions from point sources we obtained an integrated diffuse flux density of S = 640 +- 35 mJy from Coma C. We derive relations between the various observationally determined spectral indices and the spectral index of the synchrotron emissivity, which allow one to achieve a rough estimate concerning the consistency of the presently available data at different frequencies and to place constraints on the emissivity index distribution. In the halo's core region, the inferred emissivity index between 0.3 GHz and 1.4 GHz appears to be in the range 0.4 - 0.75 implying that there must be some very effective mechanism for particle acceleration operating in the intracluster medium.