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Home All issues Volume 508 / No 1 (December II 2009) A&A, 508 1 (2009) 75-92 Full HTML
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Table 3:

Radio relic properties.

Source Name 		$\alpha_{74~{\rm MHz}}^{1400~{\rm MHz}}$ spectral curvature P1.4 sizea $R_{{\rm projected}}$
    $\alpha_{74~{\rm MHz}}^{610~{\rm MHz}} - \alpha_{610~{\rm MHz}}^{1400~{\rm MHz}}$ 1024 W Hz-1 kpc kpc

VLSS J1133.7+2324 		-1.69 0.96 24.1 570  
VLSS J1431.8+1331d ... ... ... 125 175
24P73 (VLSS J2217.5+5943) -2.20 2.0 ... ... ...
MACS J0717.5+3745 -1.09b -0.02 138b 700 320
Abell 2048 (VLSS J1515.1+0424) -1.50 1.60 0.566 310 310
Abell 2256 -1.2 ... 3.95 1100 300
Abell 1240-N -1.2 ... 0.427 650 700
Abell 1240-S -1.3 ... 0.730 1250 1100
Abell 2345-E -1.3 ... 2.62 1500 890
Abell 2345-W -1.5 ... 2.83 1150 1000
Abell 13 -1.79 0.65 0.853 260 170
Abell 85 -2.30 1.36 0.322 150 430
Abell 133 -1.70 1.39 1.07 55 40
Abell 4038 -1.88 1.03 0.0983 55 35
Abell 3667 -1.1 ... 17.4 1920 1950
Abell 548b A $\sim$-2 ... 0.260 310 500
Abell 548b B <-2.0 ... 0.250 370 430
Abell 521 -1.48 ... 2.90 1000 930
Coma clusterc -1.18 ... 0.284 850 1940
Abell 2163 -1.02 ... 2.23 450 1550
Abell 2744 -1.1 ... 6.20 1620 1560
Abell S753 -2.0 ... 0.205 350 410
Abell 115 -1.1 ... 16.7 1960 1510
Abell 610 -1.4 ... 0.444 330 310
RXC J1314.4-2515-E -1.41 ... 2.08 920 685
RXC J1314.4-2515-W -1.40 ... 4.81 920 685

a Largest linear scale.
b Excluding the flux of the halo and central head-tail source (see also Bonafede et al. 2009a; van Weeren et al. 2009b).
c 1253+275.
d Blended with a nearby AGN (except in the GMRT 610 MHz image), therefore no spectral index or spectral curvature could be calculated.

Source LaTeX | All tables | In the text

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