Comparative analysis of the diffuse radio emission in the galaxy clusters A1835, A2029, and Ophiuchus

M. Murgia; F. Govoni; M. Markevitch; L. Feretti; G. Giovannini; G. B. Taylor; E. Carretti

doi:10.1051/0004-6361/200911659

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Volume 499 / No 3 (June I 2009)

A&A, 499 3 (2009) 679-695

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Table 1:

The mini-halos analyzed in this work and the basic properties of the radio images at 1.4 GHz.
Cluster	z	kpc/ $^{\prime\prime}$	Beam	$\sigma$
				mJy/beam
A1835	0.2532	3.91	53 $^{\prime\prime}$ $\times$ 53 $^{\prime\prime}$	0.025
A2029	0.0765	1.43	53 $^{\prime\prime}$ $\times$ 53 $^{\prime\prime}$	0.031
Ophiuchus	0.028	0.55	92 $^{\prime\prime}$ $\times$ 92 $^{\prime\prime}$	0.16

Column 3: Angular to linear size conversion factor; Col. 4: FWHM beam
of the radio images; Col. 5: image sensitivity.

Source LaTeX | All tables | In the text

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