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Table 5

Line kinematic properties along lines of sight.

Pointing CO [C II] H I [Ne III] Hα





MAGMA ALMA; 45′′ ALMA; 14.4′′



v(a) Δv(b) v Δv v Δv v Δv v Δv v Δv v Δv
#1 − 1.1 7.7 ... ... ... ... − 0.6 10.1 (0.9) (27.9) 2.3 22.9 ... ...
#2 5.3 6.6 4.7 5.0 5.2 5.2 5.4 6.6 (− 5.2) (37.3) (11.1) (34.8) 6.0 39.4
#3 − 0.7 8.5 2.0 2.8 2.5 2.8 (2.8) (5.2) (− 5.8) (39.8) 9.6 25.1 5.1 33.4
#4 − 0.5 7.0 − 0.1 4.9 − 0.4 5.1 1.1 6.9 0.6 38.9 (7.4) (37.4) 3.3 42.0
#5 ... ... ... ... ... ... − 10.6 4.0 − 11.3 15.9 − 3.4 7.4 − 9.7 12.4
... ... ... ... ... ... 5.7 7.0 ... ... 17.1 7.4 11.6 30.6
#6 0.8 5.0 ... ... ... ... 0.5 8.1 (− 6.3) (28.5) 4.9 22.1 − 0.1 32.5
#7 0.8 5.0 ... ... ... ... − 0.5 6.2 (− 6.3) (28.5) 4.9 22.1 − 0.1 32.5
#8 − 0.1 3.2 ... ... ... ... − 1.1 8.6 (− 3.6) (22.7) 6.6 23.1 1.1 32.6
#9 0.1 4.3 ... ... ... ... − 0.2 7.0 − 4.1 20.2 6.6 23.1 1.1 32.6
#10 − 3.9 4.5 ... ... ... ... − 4.2 4.6 1.4 23.7 ... ... − 2.0 33.8
#11 − 1.9 7.5 ... ... ... ... − 0.4 5.1 − 1.0 21.4 ... ... − 1.0 30.1
#12 − 1.1 6.1 ... ... ... ... 0.0 5.4 (0.8) (20.1) ... ... ... ...

Notes. All values are in km s−1. Values between parentheses indicate that the profile is not Gaussian (i.e., either asymmetric and/or multiple components). Only distinct components are considered. The larger FWHM observed for CO with MAGMA as compared to ALMA (45′′) is due to the low S/N of the former (Fig. 4). (a)Radial velocities in km s−1 offset from 280 km s−1. (b) Line FWHM in km s−1.

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