Table 7: Measured rotation velocities $V_{\rm rot}$ as function of projected distance (Pos) to the galaxies' centers (Pos = 0) for MS 1008-12. Galaxies are indicated by their ID with the measured emission line, respectively. See Fig. 4 for comparison.
Pos $V_{\rm rot}$ sin i cos $\delta~$
[''] [km s-1]
  B15(O[II]) A4(O[II]) B5(H$_\beta$) B3(O[II]) B16(O[II])
-1.8         +191.4 $\pm$ 72.2
-1.6   -20.4 $\pm$ 49.4      
-1.4     -99.6 $\pm$ 40.2   +175.7 $\pm$ 51.8
-1.2     -134.5 $\pm$ 19.1 +39.9 $\pm$ 80.4 -21.0 $\pm$ 98.0
-1.0 -14.3 $\pm$ 41.3 -15.5 $\pm$ 33.8 -121.1 $\pm$ 10.8 +25.9 $\pm$ 47.2 +197.0 $\pm$ 34.2
-0.8 -14.1 $\pm$ 41.9 -12.2 $\pm$ 29.4 -98.8 $\pm$ 8.3 +8.1 $\pm$ 32.4 +47.5 $\pm$ 66.0
-0.6 +0.1 $\pm$ 28.7 -11.6 $\pm$ 28.4 -84.7 $\pm$ 6.3 +19.6 $\pm$ 26.3 +52.7 $\pm$ 33.4
-0.4 -1.4 $\pm$ 19.6 -6.9 $\pm$ 25.3 -60.6 $\pm$ 6.5 +30.9 $\pm$ 24.6 +37.6 $\pm$ 24.7
-0.2 -4.4 $\pm$ 16.9 +5.6 $\pm$ 18.5 -34.7 $\pm$ 7.7 +17.8 $\pm$ 24.5 +28.5 $\pm$ 21.5
+0.0 +0.0 $\pm$ 15.4 +0.0 $\pm$ 18.3 +0.0 $\pm$ 6.3 +0.0 $\pm$ 24.0 +0.0 $\pm$ 18.8
+0.2 +7.6 $\pm$ 16.4 +8.3 $\pm$ 17.2 +21.4 $\pm$ 6.4 -23.0 $\pm$ 31.6 -24.6 $\pm$ 17.4
+0.4 +14.0 $\pm$ 17.8 +14.3 $\pm$ 14.7 +37.3 $\pm$ 5.1 -58.8 $\pm$ 38.8 -72.4 $\pm$ 27.3
+0.6 +19.7 $\pm$ 15.6 -1.9 $\pm$ 21.6 +49.3 $\pm$ 5.1 -83.6 $\pm$ 40.0 -129.0 $\pm$ 37.2
+0.8 +28.2 $\pm$ 14.7 -5.8 $\pm$ 22.3 +59.1 $\pm$ 4.3 -83.4 $\pm$ 43.4 -214.7 $\pm$ 16.1
+1.0 +35.2 $\pm$ 20.4 -18.0 $\pm$ 20.6 +65.8 $\pm$ 6.1 -93.0 $\pm$ 46.0 -183.8 $\pm$ 29.6
+1.2 +53.2 $\pm$ 22.4 -24.0 $\pm$ 26.8 +79.5 $\pm$ 6.5 -95.4 $\pm$ 44.7  
+1.4 +73.6 $\pm$ 21.3 +16.1 $\pm$ 43.9 +87.0 $\pm$ 10.2    
+1.6 +85.8 $\pm$ 22.4        
+1.8 +74.4 $\pm$ 12.8        
+2.0 +64.9 $\pm$ 11.0        


Source LaTeX | All tables | In the text