Table A.2
Locations of MIVC± candidates with angular sizes Ω smaller than one GASS beam.
l | b | vLSR | ϵIVC |
![]() |
FWHM | Ω | Stot | No. | Designation |
[deg] | [deg] | [km s-1] | [10-26 cm2] | [1020 cm-2] | [km s-1] | [deg2] | [Jy km s-1] | ||
|
|||||||||
vLSR< −20 km s-1 | |||||||||
|
|||||||||
70.0 | 54.8 | −22.7 | 0.58 ± 0.02 | 0.42 ± 0.13 | 3.8 | 0.012 | 12.2 | 28 | |
84.3 | −37.2 | −46.4 | 0.98 ± 0.21 | 0.96 ± 0.06 | 4.6 | 0.003 | 16.0 | 55 | |
85.2 | −36.8 | −48.8 | 0.13 ± 0.02 | 4.78 ± 0.28 | 4.6 | 0.056 | 25.8 | 49 | |
86.1 | −38.1 | −42.5 | 0.29 ± 0.01 | 4.24 ± 0.18 | 5.0 | 0.018 | 16.3 | 23 | |
87.2 | 57.8 | −38.9 | 0.21 ± 0.01 | 1.21 ± 0.31 | 4.3 | 0.041 | 5.0 | 17 | |
93.1 | 23.2 | −35.6 | 0.81 ± 0.02 | 0.59 ± 0.09 | 4.7 | 0.068 | 12.7 | 7 | |
96.0 | 25.1 | −35.1 | 0.57 ± 0.01 | 0.62 ± 0.19 | 4.4 | 0.015 | 19.8 | 13 | |
96.2 | −30.6 | −53.0 | −0.26 ± 0.07 | 5.71 ± 1.15 | 4.7 | 0.021 | 6.6 | 60 | |
98.1 | 21.9 | −47.3 | 0.35 ± 0.05 | 3.07 ± 0.30 | 3.8 | 0.074 | 19.8 | 40 | |
100.1 | 27.8 | −51.1 | 0.30 ± 0.01 | 1.48 ± 0.32 | 4.6 | 0.009 | 29.4 | 24 | |
105.1 | 34.0 | −52.5 | 0.47 ± 0.02 | 0.90 ± 0.20 | 3.5 | 0.029 | 16.2 | 22 | |
106.1 | −23.8 | −35.8 | 0.00 ± 0.00 | 0.00 ± 0.00 | 4.3 | 0.009 | 30.0 | 58 | |
107.0 | −24.4 | −56.2 | 0.00 ± 0.00 | 0.00 ± 0.00 | 3.4 | 0.018 | 41.7 | 59 | |
108.3 | 35.5 | −70.7 | 0.15 ± 0.01 | 1.78 ± 0.45 | 4.5 | 0.032 | 18.1 | 41 | |
108.7 | −33.4 | −53.4 | 0.69 ± 0.01 | 0.54 ± 0.10 | 4.7 | 0.032 | 8.1 | 6 | |
108.7 | 25.4 | −28.8 | 0.45 ± 0.09 | 3.24 ± 1.01 | 4.9 | 0.074 | 18.0 | 46 | |
112.2 | 37.6 | −36.1 | 0.78 ± 0.02 | 0.43 ± 0.14 | 4.7 | 0.015 | 21.1 | 20 | |
113.6 | 37.3 | −54.4 | 0.74 ± 0.01 | 0.48 ± 0.13 | 4.4 | 0.024 | 24.6 | 10 | |
113.6 | 34.0 | −79.3 | 0.29 ± 0.02 | 0.76 ± 0.36 | 4.3 | 0.029 | 17.6 | 27 | |
113.7 | 34.9 | −71.8 | 0.39 ± 0.01 | 0.61 ± 0.21 | 4.8 | 0.003 | 18.5 | 43 | |
114.0 | 34.6 | −76.7 | 0.45 ± 0.01 | 0.53 ± 0.18 | 4.7 | 0.059 | 20.7 | 9 | |
116.2 | 56.6 | −65.9 | 0.43 ± 0.03 | 0.61 ± 0.23 | 4.2 | 0.038 | 6.1 | 25 | |
122.4 | 30.0 | −26.6 | 4.06 ± 0.26 | 2.34 ± 0.07 | 4.8 | 0.027 | 20.4 | 34 | |
126.3 | −25.6 | −58.3 | 1.08 ± 0.02 | 0.53 ± 0.08 | 4.8 | 0.027 | 32.1 | 11 | |
127.0 | −28.3 | −21.2 | 0.81 ± 0.02 | 0.66 ± 0.13 | 4.9 | 0.015 | 28.3 | 16 | |
127.3 | −26.4 | −36.6 | 0.97 ± 0.02 | 0.22 ± 0.10 | 4.6 | 0.074 | 25.8 | 3 | |
130.2 | 39.3 | −20.8 | −0.84 ± 0.04 | 0.40 ± 0.13 | 4.5 | 0.009 | 12.6 | 62 | |
130.4 | 51.3 | −47.6 | 0.39 ± 0.02 | 0.73 ± 0.22 | 4.4 | 0.080 | 72.2 | 19 | IVC 135 |
141.8 | 41.1 | −48.5 | 2.30 ± 0.03 | 0.91 ± 0.07 | 4.5 | 0.044 | 23.2 | 4 | |
144.5 | 42.2 | −51.0 | 0.51 ± 0.05 | 2.89 ± 0.57 | 4.6 | 0.009 | 17.6 | 52 | |
150.7 | 40.3 | −59.2 | 0.59 ± 0.07 | 3.63 ± 0.45 | 4.3 | 0.056 | 38.4 | 39 | |
151.1 | 32.6 | −49.4 | 0.94 ± 0.04 | 0.65 ± 0.14 | 4.0 | 0.012 | 22.4 | 33 | |
152.3 | 39.7 | −52.5 | 1.67 ± 0.09 | 0.70 ± 0.16 | 3.2 | 0.003 | 52.6 | 50 | |
154.6 | 38.7 | −59.8 | 1.33 ± 0.08 | 1.97 ± 0.27 | 3.8 | 0.015 | 59.0 | 37 | |
163.0 | 34.9 | −59.1 | 0.89 ± 0.01 | 0.39 ± 0.09 | 3.8 | 0.062 | 34.2 | 1 | |
176.5 | 27.8 | −25.5 | 0.23 ± 0.02 | 1.07 ± 0.49 | 4.1 | 0.015 | 38.1 | 44 | |
202.2 | 53.8 | −20.9 | 0.73 ± 0.01 | 0.37 ± 0.09 | 4.8 | 0.018 | 49.6 | 8 | |
204.0 | 39.5 | −37.1 | 0.82 ± 0.02 | 0.50 ± 0.10 | 3.6 | 0.009 | 9.1 | 18 | |
206.2 | 48.6 | −39.8 | 1.31 ± 0.03 | 0.29 ± 0.05 | 4.1 | 0.003 | 15.7 | 29 | |
206.5 | 48.6 | −43.2 | 1.43 ± 0.02 | 0.24 ± 0.04 | 4.7 | 0.080 | 14.2 | 2 | |
209.0 | 49.6 | −47.6 | 0.22 ± 0.02 | 1.24 ± 0.33 | 4.5 | 0.032 | 12.1 | 42 | |
209.3 | 49.3 | −47.6 | 0.23 ± 0.02 | 1.45 ± 0.37 | 4.5 | 0.018 | 10.5 | 48 | |
211.8 | 44.8 | −33.1 | 0.99 ± 0.02 | 0.35 ± 0.10 | 3.2 | 0.003 | 25.3 | 31 | |
213.2 | 61.9 | −35.6 | 0.82 ± 0.02 | 0.73 ± 0.11 | 4.5 | 0.009 | 14.7 | 21 | IVC 210 |
213.5 | 39.0 | −38.5 | −0.12 ± 0.02 | 2.12 ± 0.69 | 5.0 | 0.038 | 3.7 | 61 | |
218.6 | 41.4 | −33.8 | 0.31 ± 0.03 | 1.34 ± 0.40 | 4.6 | 0.065 | 2.1 | 30 | |
252.9 | 76.1 | −25.8 | 0.84 ± 0.02 | 1.11 ± 0.10 | 4.8 | 0.029 | 42.6 | 15 | |
254.4 | 77.1 | −25.8 | 0.66 ± 0.02 | 0.45 ± 0.15 | 5.0 | 0.053 | 54.6 | 12 | |
256.1 | 79.1 | −29.1 | 0.20 ± 0.04 | 1.82 ± 0.60 | 3.9 | 0.006 | 39.3 | 54 | |
256.8 | 73.1 | −30.6 | 0.82 ± 0.06 | 3.09 ± 0.31 | 3.7 | 0.003 | 87.5 | 53 | |
258.3 | 78.1 | −28.6 | 0.10 ± 0.03 | 4.96 ± 1.37 | 2.8 | 0.080 | 45.7 | 51 | |
258.7 | 76.0 | −28.5 | 1.11 ± 0.02 | 0.39 ± 0.09 | 4.4 | 0.050 | 69.0 | 5 | |
259.2 | 49.7 | −29.4 | 0.38 ± 0.01 | 0.70 ± 0.22 | 4.9 | 0.009 | 16.4 | 35 | |
260.5 | 50.3 | −23.5 | 0.35 ± 0.02 | 0.90 ± 0.30 | 4.8 | 0.029 | 15.9 | 26 | |
269.4 | 81.7 | −29.2 | 0.54 ± 0.04 | 0.94 ± 0.27 | 4.9 | 0.024 | 41.7 | 36 | |
271.0 | 75.4 | −39.9 | 0.09 ± 0.01 | 5.69 ± 0.82 | 4.1 | 0.029 | 58.2 | 47 | |
279.1 | 85.2 | −28.3 | 0.16 ± 0.03 | 2.11 ± 0.45 | 4.3 | 0.062 | 55.1 | 45 | |
284.4 | 52.6 | −29.1 | 0.69 ± 0.02 | 1.11 ± 0.22 | 3.6 | 0.003 | 24.7 | 38 | |
286.2 | 52.6 | −23.7 | 1.35 ± 0.03 | 0.59 ± 0.10 | 3.6 | 0.021 | 18.6 | 14 | G 288.4+53.2 |
303.2 | −23.9 | −27.7 | 0.00 ± 0.00 | 0.00 ± 0.00 | 4.4 | 0.047 | 15.9 | 56 | |
312.5 | 54.6 | −48.0 | 0.75 ± 0.03 | 0.44 ± 0.12 | 3.8 | 0.012 | 47.4 | 32 | |
316.0 | −20.6 | −26.0 | 0.00 ± 0.00 | 0.00 ± 0.00 | 4.9 | 0.006 | 76.1 | 57 | |
|
|||||||||
vLSR> +20 km s-1 | |||||||||
|
|||||||||
25.2 | −19.8 | 25.1 | 0.00 ± 0.00 | 0.00 ± 0.00 | 5.0 | 0.021 | 79.6 | 6 | |
25.5 | −20.8 | 23.0 | 0.00 ± 0.00 | 0.00 ± 0.00 | 4.8 | 0.038 | 103.9 | 5 | |
254.1 | −21.7 | 36.8 | 0.61 ± 0.03 | 1.33 ± 0.34 | 4.3 | 0.003 | 57.3 | 4 | |
254.3 | −23.8 | 22.9 | 0.25 ± 0.01 | 1.77 ± 0.41 | 4.9 | 0.029 | 38.4 | 1 | |
290.2 | 37.3 | 30.5 | 0.40 ± 0.02 | 1.94 ± 0.21 | 4.0 | 0.006 | 3.1 | 3 | |
293.0 | 37.6 | 29.0 | 1.06 ± 0.05 | 0.67 ± 0.04 | 4.9 | 0.006 | 2.0 | 2 |
Notes. The columns give the Galactic longitude l and latitude b, the radial velocity vLSR, the fitted IVC dust emissivity ϵIVC and its error, the peak H2 column density and its error, the line width FWHM, the angular size Ω, the total H i flux Stot within −100 km s-1 ≤ vLSR ≤ −20 km s-1 or + 20 km s-1 ≤ vLSR ≤ +100 km s-1, the rank for the samples with negative or positive LSR velocities as determined by the significance S (Eq. (4)), and the MIVC designation if it is a known cloud. If there are spectral components towards a single candidate that are separated by more than 10 km s-1, then we give these two different spectral components with individual centre velocities and line widths. If ϵIVC and
are both 0.00 ± 0.00, then the candidate is not fitted because either the LVC and IVC H i column densities within 2° × 2° around the candidate are higher than 4 × 1020 cm-2.
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