Open Access

Table B.1.

Impact of an alternative definition of offsets.

θCO − Hα σ ρ ΩP
peak 2nd p. weight peak 2nd p. weight peak 2nd p. weight peak 2nd p. weight
IC1954 206 176 137 1040 1166 465 0.29 0.16 0.18 32.7 33.6 28.8
NGC0628 236 220 154 948 1304 333 0.15 0.02 0.20 31.7 32.7 32.4
NGC1300 457 -90 426 3587 2615 2272 -0.01 -0.11 -0.05 23.0 23.1 23.0
NGC1385 265 54 189 1040 1125 663 0.31 0.14 0.27 26.1 26.4 25.9
NGC1512 -402 -778 -654 3083 3317 3991 0.19 -0.02 0.23 21.4 21.4 21.3
NGC1566 403 451 330 1064 1119 642 0.56 0.44 0.50 25.0 24.8 24.0
NGC1672 106 -31 -29 582 565 222 -0.21 -0.19 -0.41 15.1 15.0 14.4
NGC2090 33 124 1 596 600 138 -0.14 -0.08 -0.12 147.2 -218.7 97.9
NGC2283 201 93 3 752 888 307 0.32 0.33 0.24 28.2 31.9 34.0
NGC2566 737 73 -16 5110 6712 3456 0.01 0.01 0.20 16.1 16.2 16.2
NGC2835 -11 -10 -96 852 1222 622 0.21 0.14 0.18 29.3 29.3 29.8
NGC2997 250 358 494 2135 1557 1509 -0.01 0.04 0.11 28.2 28.1 28.0
NGC3507 146 134 -119 1757 2391 717 0.23 0.12 -0.21 27.6 22.8 23.1
NGC3627 176 90 201 962 984 371 0.29 0.34 0.40 26.6 29.6 19.1
NGC4254 377 271 181 1093 1086 603 0.14 0.04 0.03 15.2 2.4 97.0
NGC4303 691 596 112 2070 2393 663 0.40 0.13 0.24 34.8 35.3 35.3
NGC4321 409 151 398 1738 1243 537 0.09 0.08 0.21 22.5 22.7 15.7
NGC4535 0 -27 208 937 1030 793 -0.29 -0.09 -0.29 27.2 27.2 27.1
NGC4548 254 53 31 896 743 269 -0.03 -0.15 -0.51 36.7 36.8 40.8
NGC4731 188 194 115 575 653 438 0.23 0.15 0.38 25.1 26.0 24.8
NGC5194 399 155 456 1111 1800 1961 -0.34 -0.07 0.04 61.5 43.8 43.4
NGC5248 72 47 -66 798 679 476 0.21 0.20 0.21 25.3 25.2 26.1
NGC5643 282 134 -119 2114 2391 717 0.00 0.12 -0.21 35.4 22.8 23.1
NGC6744 1 134 -119 1051 2391 717 0.21 0.16 0.18 23.0 22.9 23.2

Notes. Mean CO-Hα offsets, their scatter, the strength of the θ–Ω correlation (Spearman rank ρ) and the implied pattern speed (ΩP) for alternative definitions of offsets. ‘Peak’ represents our nominal measurement, based on the peak emission in CO and Hα (see Fig. 2); ‘2nd peak’ considers instead the azimuthal bin corresponding to the second brightest peak in CO and Hα for each spiral arm at each radius; finally, ‘weighted’ considers the mean azimuth weighted by CO and Hα luminosity for each spiral at each radius.

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