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Table A.1.

Physical properties of the filaments

ID l1 b1 l2 b2 vlsr d Len. Le2e Lmst w Aspect Δv Slope Mass Lum. L/M T N70 Ncl Linearity θ z Arm Pv P v P cl $ \frac{P_{\mathrm{v}}}{P_{\mathrm{cl}}} $
° ° ° ° km s $ \rm \frac{km}{s} $ kpc ° pc pc pc ratio km s $ \rm \frac{km}{s} $ km / s pc $ \rm \frac{km/s}{pc} $ M L L M $ \frac{L_\odot}{M_\odot} $ K ° pc pc
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13) (14) (15) (16) (17) (18) (19) (20) (21) (22) (23) (24) (25) (26)
F1 10.17 -0.36 10.18 -0.35 19.5 13.6 0.135 31.9 33.0 2.3 14.1 3.2 0.08 3.5E+04 8.7E+05 24.83 15.5 3 5 12.2 71 -100 Perseus
F2 12.0 -0.42 12.05 -0.42 45.3 12.0 0.187 39.2 39.5 2.4 16.4 4.3 -0.12 6.1E+03 5.6E+03 0.9 14.5 3 5 20.9 10 -87
F3 14.62 0.33 14.61 0.38 26.6 2.7 0.144 6.8 7.0 0.4 15.8 1.4 0.07 7.6E+02 2.6E+03 3.37 16.6 4 5 13.5 68 34 1.3 0.7
F4 18.07 0.55 18.07 0.57 23.3 13.7 0.09 21.5 22.0 2.1 10.6 1.2 0.06 2.4E+04 3.9E+03 0.16 12.4 0 5 10.5 89 125 Perseus 5.5 1.0
F5 21.7 -0.28 21.71 -0.26 85.3 10.6 0.149 27.6 28.1 2.2 12.9 1.7 -0.06 1.1E+04 3.3E+03 0.3 12.3 1 5 10.1 51 -53 Scu-Cen 7.5 1.1
F6 26.19 0.59 26.2 0.6 105.4 9.3 0.106 17.2 17.6 1.5 11.6 0.4 -0.01 1.4E+03 2.4E+03 1.73 16.2 0 5 12.3 74 98 4.5 1.0
F7 26.46 0.72 26.5 0.71 48.0 3.1 0.158 8.5 8.6 0.4 22.2 0.8 -0.01 7.3E+02 3.0E+03 4.16 15.3 2 5 23.8 17 59 2.5 1.2
F8 28.83 -0.33 28.83 -0.31 100.8 9.1 0.121 19.2 19.9 1.7 12.1 0.4 0.01 1.3E+04 2.0E+03 0.16 10.9 1 5 14.5 85 -49 8.45 1.7
F9 29.8 -0.83 29.81 -0.83 82.8 4.7 0.152 12.5 13.1 0.7 19.3 1.9 0.06 1.9E+03 2.8E+02 0.15 11.9 0 7 11.7 18 -50 Scu-Cen 2.3 1.1
F10 30.74 -0.89 30.73 -0.86 80.3 4.5 0.134 10.6 10.8 0.7 14.5 1.1 -0.1 1.7E+03 2.5E+02 0.15 11.4 1 5 13.3 56 -54 2.8 1.0
F11 32.74 -0.08 32.75 -0.06 36.9 11.7 0.154 31.5 32.8 1.5 22.2 1.8 -0.03 9.2E+03 2.0E+05 21.6 20.7 7 7 17.8 82 -22 Sag-Car 7.0 1.3
F12 36.88 -0.5 36.88 -0.47 59.7 9.8 0.099 16.8 17.2 1.3 13.0 2.0 0.09 1.0E+04 2.5E+04 2.5 12.4 2 5 10.1 79 -78 Sag-Car
F13 40.02 -0.12 40.02 -0.09 83.6 4.5 0.221 17.3 18.6 0.9 21.1 1.6 0.06 1.7E+03 2.9E+03 1.76 11.7 1 7 10.6 87 3 2.5 0.8
F14 48.6 0.36 48.61 0.35 35.9 8.6 0.102 15.3 15.7 1.6 10.0 1.4 0.1 4.5E+03 2.0E+03 0.44 13.1 1 5 10.6 40 72 3.8 1.0
F15 56.23 0.05 56.24 0.05 -4.2 9.6 0.113 19.0 21.3 1.2 17.9 1.7 0.07 7.6E+03 3.0E+04 3.95 14.0 4 6 12.1 22 27 Perseus
F16 60.38 0.18 60.37 0.23 20.3 6.4 0.128 14.3 14.4 1.5 9.7 1.1 -0.11 5.5E+02 7.3E+02 1.33 16.5 1 5 18.2 77 40
F17 66.1 0.38 66.09 0.38 16.0 4.9 0.136 11.7 11.9 0.7 17.6 2.7 -0.21 1.2E+03 1.4E+02 0.11 11.4 0 5 10.9 59 51
F18 70.85 -0.01 70.87 -0.01 9.1 1.2 0.147 3.2 3.3 0.3 13.0 1.4 -0.01 9.0E+01 1.1E+01 0.12 11.1 0 5 10.4 54 24
F19 71.83 1.22 71.85 1.22 15.2 1.9 0.103 3.4 3.5 0.3 10.3 0.9 -0.29 2.4E+02 4.2E+01 0.17 11.0 2 5 11.5 16 66
F20 80.66 1.28 80.68 1.26 -64.1 9.1 0.133 21.0 21.6 1.4 15.6 2.1 -0.11 2.3E+03 6.2E+03 2.73 17.3 5 6 10.6 22 232
F21 103.68 0.43 103.68 0.44 -61.5 4.2 0.108 8.0 8.1 0.5 15.7 1.9 0.24 2.8E+02 9.5E+02 3.38 14.5 3 5 11.2 51 61
F22 182.03 -0.23 182.02 -0.22 -10.4 4.4 0.146 11.1 11.7 0.7 17.1 0.8 -0.09 2.5E+03 2.1E+02 0.08 9.4 4 7 11.1 68 21
F23 189.25 0.71 189.24 0.73 10.4 2.8 0.16 7.8 8.0 0.4 19.1 1.1 -0.15 3.5E+02 3.4E+01 0.1 10.0 1 6 14.8 69 68 Perseus
F24 224.02 -1.67 224.03 -1.63 17.6 1.3 0.124 2.8 2.8 0.2 14.5 0.0 0.0 4.8E+01 4.4E+01 0.92 12.6 3 5 12.2 78 -9
F25 225.44 -0.24 225.48 -0.23 16.6 1.2 0.191 3.9 4.0 0.3 15.1 0.4 -0.04 1.4E+02 4.5E+00 0.03 8.6 0 5 19.4 15 23
F26 239.68 -0.8 239.68 -0.81 65.0 5.2 0.094 8.6 9.1 0.6 15.4 0.3 -0.04 2.1E+02 9.6E+01 0.47 13.4 2 5 12.3 7 -37 Perseus
F27 283.78 -0.38 283.78 -0.37 -2.6 5.5 0.091 8.8 9.2 1.3 7.2 0.0 0.0 7.8E+02 2.2E+03 2.82 20.0 1 5 11.7 36 -13 Sag-Car
F28 290.77 -1.43 290.77 -1.41 9.3 6.9 0.138 16.5 16.8 1.0 16.1 1.9 -0.15 9.2E+02 6.3E+03 6.86 13.8 1 5 15.9 69 -153
F29 305.22 0.5 305.26 0.49 -46.7 4.8 0.16 13.4 13.8 0.8 18.1 2.2 -0.14 2.6E+03 9.2E+02 0.35 12.8 3 6 10.7 14 63 2.6 0.9
F30 305.41 0.71 305.45 0.74 -46.5 4.9 0.257 22.1 23.4 0.7 32.9 1.5 0.06 2.9E+03 9.1E+02 0.32 11.7 2 9 10.4 31 78
F31 319.97 0.56 319.98 0.56 -40.1 2.5 0.121 5.3 5.5 0.5 11.8 1.2 0.03 2.8E+02 4.3E+01 0.15 10.9 0 5 11.4 10 45
F32 323.69 0.63 323.72 0.63 -46.9 10.6 0.134 24.8 26.6 1.9 14.4 1.5 0.04 5.3E+03 4.1E+04 7.7 16.9 3 6 11.3 2 124
F33 324.16 -0.66 324.15 -0.62 -33.3 9.6 0.183 30.6 30.9 2.0 15.6 1.2 0.0 5.2E+03 1.1E+03 0.22 12.4 0 5 13.4 90 -108
F34 328.81 0.07 328.81 0.07 -32.9 12.1 0.062 13.1 13.2 1.7 7.9 2.6 0.26 6.1E+03 2.6E+04 4.22 16.0 5 5 15.4 53 15 3.3 1.0
F35 338.56 0.22 338.58 0.21 -36.5 2.8 0.12 5.8 5.8 0.4 14.7 2.7 -0.11 7.7E+02 4.9E+03 6.38 17.8 4 5 17.6 3 30 Nor-Out 1.85 1.3
F36 338.82 -0.47 338.87 -0.48 -38.8 2.9 0.367 18.3 20.1 0.4 48.0 3.5 0.01 3.5E+03 4.2E+02 0.12 10.4 7 11 10.2 8 -4 Scu-Cen 2.0 1.0
F37 340.79 0.57 340.79 0.59 -124.9 9.4 0.144 23.5 24.2 1.6 14.9 0.8 -0.03 5.3E+03 1.6E+03 0.31 12.8 0 5 11.0 62 94
F38 342.93 -0.77 342.95 -0.75 -26.7 2.0 0.118 4.1 4.1 0.4 9.7 0.7 -0.14 1.4E+03 6.2E+01 0.04 8.9 1 5 15.8 44 -6 Nor-Out 1.14 1.1
F39 346.02 -0.02 346.06 -0.03 -80.3 10.8 0.189 35.7 36.8 1.4 25.8 2.8 -0.08 1.2E+04 6.4E+04 5.52 16.0 5 6 10.2 7 -1 4.0 0.5
F40 348.04 -0.44 348.05 -0.43 -94.7 6.0 0.104 10.9 11.1 1.1 10.3 2.1 -0.08 6.4E+03 4.3E+04 6.71 15.6 4 5 12.2 2 -33 3.0 1.1
F41 348.73 -0.29 348.77 -0.26 -19.3 2.2 0.184 7.1 7.1 0.4 16.1 0.7 -0.11 2.9E+02 1.3E+02 0.44 12.1 1 5 12.9 19 9 1.6 0.9
F42 352.62 -1.08 352.63 -1.07 -0.6 16.3 0.069 19.6 20.0 1.1 18.5 1.7 -0.09 5.1E+04 1.4E+06 27.86 21.9 5 5 12.7 51 -321 Sag-Car
Min -177.97 -1.67 -124.9 1.2 0.062 2.8 2.8 0.2 7.2 0.0 0.00 4.8E+01 4.5E+00 0.03 8.6 0.0 5.0 10.1 1.9 -320.5 1.1 0.5
Max 103.68 1.28 105.4 16.3 0.367 39.2 39.5 2.4 48.0 4.3 0.29 5.1E+04 1.4E+06 27.86 21.9 7.0 11.0 23.8 90.0 232.2 8.5 1.7
Avg -8.92 -0.05 4.8 6.7 0.142 15.5 16.0 1.1 16.2 1.5 0.08 5.8E+03 6.6E+04 3.47 13.7 2.2 5.6 13.1 44.5 6.8 3.6 1.0
Med 1.40 -0.05 9.9 5.4 0.135 13.9 14.1 1.0 15.3 1.5 0.07 2.1E+03 2.0E+03 0.69 12.8 2.0 5.0 12.2 51.2 18.0 2.8 1.0
Std 66.76 0.66 54.0 4.0 0.053 9.4 9.7 0.6 7.0 0.9 0.07 9.9E+03 2.6E+05 6.41 3.1 2.0 1.2 3.2 29.3 88.2 2.1 0.2
Skewness -0.9 -0.2 -0.1 0.5 2.1 0.7 0.7 0.5 2.7 0.7 1.2 3.3 4.7 2.9 0.7 0.8 3.0 1.6 0.0 -1.0 1.1 0.8
Kurtosis 0.5 -0.1 -0.3 -0.8 7.5 -0.1 -0.3 -0.9 10.4 0.8 1.4 12.1 22.5 8.1 0.3 -0.2 10.2 2.3 -1.5 4.1 0.4 3.2

Notes. Col. (1) Assigned filament ID. Cols. (2-5) Galactic coordinates of the two end-to-end clumps. Statistics (last rows) are computed by converting l to [-180, 180] deg. Col. (6) Mean LSR velocity of the clumps in a filament. Col. (7) Distance (Sect. 3.1). Cols. (8-9) End-to-end length, in angular and physical units. Col. (10) Curved length following the MST, i.e., connecting the clumps. Col. (11) Width, the diameter of the largest clump in the filament. Col. (12) Aspect ratio, length divided by width. Col. (13) Difference between the min. and max. velocity of the clumps in a filament. Col. (14) Slope by fitting clump velocity along the filament (Sect. 3.1). Statistics (last rows) are given for |Slope|. Cols. (15-16) Sum of clump mass/luminosity, which gives lower limit for filament mass/luminosity (Sect. 3.1). Col. (17) Luminosity/mass ratio. Col. (18) Mean dust temperature of the clumps. Col. (19-20) Number of 70 μm sources, and number of HiGAL clumps. Col. (21) Linearity, as defined in Paper I and refined in Paper II (Sect. 2). Col. (22) Angle between filament and Galactic mid-plane. Col. (23) Height from the Galactic mid-plane. Col. (24) Associated spiral arm, if any. Col. (25) Velocity oscillation period determined from PV analysis (Sect. 3.3). Col. (26) Ratio of velocity period to density period (mean separation between clumps, Sect. 3.3). The last rows list statistics of the parameters. Skewness (S) measures symmetry of a distribution. S = 0 means symmetric distribution, negative and positive S mean asymmetric tails with lower and higher values around the mean, respectively. Kurtosis (K) measures how spread the distribution is compared to a normal distribution. A normal distribution has K = 0. K > 0 means the distribution is more centrally peaked than normal distribution, and K < 0 is flatter. Cross-match: Six filaments (F1, 3, 7, 35, 36, 40) (partially) overlap with previously known filaments. F1 is a small part of an X-shaped filament (F5 in Paper I and F7 in Paper II). F7 is part of the X-shaped Herschel cold filament CFG26 (Wang et al. 2015). F36 is the central and linear part of the well kown S-shaped Nessie filament (Jackson et al. 2010; Wang et al. 2015). F40 is partly overlapped with F90 in Paper II. F3, F35, F36 are part of G014.478+0.736, G338.528+0.214, G338.680-0.455 in Li et al. (2016), respectively.

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