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Table 3:

Characteristics of split RM profiles in galaxy cores.
Galaxy RA Dec Nucleus Feature $\phi $ $P(\phi)$ $Q(\phi)$ $U(\phi)$ $\chi(\phi)$
ID J2000 J2000 type no. [ ${}~{\rm rad~m}^{-2}$] [$\mu$Jy] [$\mu$Jy] [$\mu$Jy] [deg]
NGC 2903 09 32 09.8 21 30 00 H 1 -93 143.0 -102.4 18.3 84.9
NGC 2903       2 +70 276.0 141.3 -245.6 -30.0
NGC 3627 11 20 15.8 12 59 26 T2/S2 1 -133 144.0 111.7 -39.5 -9.7
NGC 3627       2 +55 153.0 146.8 44.1 8.4
NGC 4321 12 22 54.9 15 49 21 T2 1 -103 191.0 -149.6 -40.6 -82.4
NGC 4321       2 +150 135.0 9.6 -136.6 -43.0
NGC 4631 12 42 07.7 32 32 26 H 1 -108 88.0 -57.5 -60.1 -66.9
NGC 4631       2 +73 87.0 33.1 -74.9 -33.1
NGC 4736 12 50 53.1 41 07 14 L2 1 -128 178.0 268.3 -63.1 -6.6
NGC 4736       2 +135 184.0 164.6 -66.5 -11.0
NGC 5194 13 29 52.7 47 11 47 S2 1 -28 91.0 12.7 -4.1 -8.9
NGC 5194       2 +128 97.0 73.7 9.3 3.6
NGC 6946 20 34 52.3 60 09 22 H 1 -208 122.0 -53.1 -45.4 -69.7
NGC 6946       2 +15 74.0 26.2 50.9 31.4
NGC 6946       3 +233 110.0 68.3 -30.4 -12.0

Source LaTeX | All tables | In the text

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