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Table 1

Lines of sight with detections of OH 1665/1667 MHz absorption.

Name RA (J2000) Dec (J2000) Fc (20′′) Fc(46′′) Ext. α OH velocities Ass. H II H II-region
(°′′′) [Jy beam−1] [Jy beam−1] [km s−1]
G14.490+0.021 18 16 46.666 −16 20 33.15 0.2 0.2 1 +0.0 (23.1) (1) G014.489+00.020
G14.996−0.738 18 20 33.756 −16 15 22.46 1.1 3.4 1 +0.7 21.8 1 G015.035−00.677; M17; S45
G15.033−0.679 18 20 25.129 −16 11 43.00 3.4 13.4 1 +0.7 12.9 1 G015.035−00.677; M17; S45
G18.148−0.283 18 25 01.009 −13 15 30.78 0.4 1.1 1 +0.1 56.4 1 G018.144−00.286
G18.303−0.390 18 25 42.284 −13 10 18.26 0.8 1.1 1 +0.4 (27.2), 32.2, (36.2) (1), 1, (1) G018.305−00.391
G19.075−0.288 18 26 48.526 −12 26 28.66 0.4 0.7 1 +0.4 64.6 1 G019.066−00.281; W39
G21.347−0.629 18 32 20.815 −10 35 11.37 1.0 1.0 0 +0.0 56.1 0
G21.874+0.007 18 31 02.524 −09 49 30.49 0.5 0.6 1 +0.3 21.8 1 G021.870+00.010
G23.956+0.150 18 34 25.303 −07 54 46.37 0.9 1.3 1 +0.6 80.0 1 G023.956+00.152
G25.396+0.033 18 37 30.623 −06 41 16.38 0.3 0.4 1 +0.4 −12.1 1 G025.396+00.034
G25.397−0.141 18 38 08.202 −06 45 58.85 1.6 2.4 1 +0.8 67.1, 94.5 1, 1 G025.383−00.177
G26.609−0.212 18 40 37.495 −05 43 19.00 0.2 0.2 1 +0.3 −33.2 1 G026.610−00.212a
G27.563+0.084 18 41 19.379 −04 44 17.57 0.1 0.1 1 +0.2 86.0 1 G027.562+00.084
G28.806+0.174 18 43 16.959 −03 35 28.97 0.3 0.7 1 +0.1 79.8, 103.5 0, 1 G028.801+00.174
G29.935−0.053 18 46 09.525 −02 41 27.54 0.5 1.2 1 +0.1 7.0, 50.6, 68.0, 98.9 0, 0, 0, 1 G029.945−00.039; G29
G29.957−0.018 18 46 04.241 −02 39 19.25 1.4 2.0 1 +0.9 8.0, 99.8 0, 1 G029.945−00.039; G29
G30.535+0.021 18 46 59.359 −02 07 26.40 0.5 0.7 1 +0.6 (43.7, 49.4), 91.6 (1, 1), 1 G030.539+00.024
G30.720−0.083* 18 47 41.713 −02 00 23.48 0.4 0 +1.0 93.6 1 G030.782−00.028; W43
G30.783−0.028 18 47 36.898 −01 55 30.26 1.3 3.9 1 +0.3 77.9, 81.9, 87.1 1, 1, 1 G030.782−00.028; W43
92.1, 98.6 1, 1
G30.854+0.151 18 47 06.546 −01 46 49.14 0.1 0.3 1 −0.1 95.4 1 G030.852+00.149a
G31.242−0.110 18 48 44.821 −01 33 14.65 0.4 0.5 1 +0.5 19.6, 79.2, 83.7 1, 0, 0 G031.239−00.108
G31.388−0.383 18 49 59.195 −01 32 56.04 1.2 1.2 0 −0.9 18.1 0
G32.151+0.132 18 49 32.499 −00 38 05.79 0.4 0.5 1 +0.4 93.8 1 G032.160+00.130
G32.272−0.226 18 51 02.358 −00 41 24.22 0.3 0.3 1 +0.2 22.6 1 G032.272−00.226
G32.798+0.190 18 50 31.084 −00 01 56.81 1.2 1.5 1 +1.0 12.8 1 G032.960+00.276
G32.928+0.607 18 49 16.315 00 16 23.85 0.2 0.3 1 +0.4 (−33.9) (1) G032.928+00.607
G33.915+0.110 18 52 50.381 00 55 29.56 0.6 0.8 1 +0.5 (95.3, 101.5), 106.3 (1, 1), 1 G033.910+00.110
G34.132+0.471 18 51 57.102 01 16 58.86 0.4 0.5 1 +0.2 33.8 1 G034.133+00.471
G35.467+0.139 18 55 34.169 02 19 11.16 0.2 0.3 1 +0.6 77.0 1 G035.470+00.140
G37.764−0.215 19 01 02.118 04 12 03.76 0.4 1.1 1 +0.1 63.4 1 G037.760−00.200
G37.874−0.399 19 01 53.641 04 12 52.52 1.3 1.8 1 +0.5 61.0 1 G037.870−00.400; W47
G38.876+0.308 19 01 12.538 05 25 44.28 0.2 0.2 0 +0.8 −16.3 1 G038.875+00.308
G39.565−0.040 19 03 43.340 05 52 55.41 0.4 0.5 0 −0.9 23.2 0
G39.883−0.346 19 05 24.156 06 01 28.52 0.2 0.3 0 +0.8 56.9 1 G039.883−00.346
G41.741+0.097 19 07 15.655 07 52 42.12 0.3 0.3 1 +0.3 14.2 1 G041.740+00.100
G42.027−0.604 19 10 18.252 07 48 32.39 0.3 0.4 1 −1.0 65.1 0
G45.454+0.060 19 14 21.188 11 09 12.92 1.4 2.9 1 +0.4 56.0, 59.4, 64.9 1, 1, 1 G045.454+00.059; K47
G49.206−0.342 19 23 00.834 14 16 50.73 0.8 2.3 1 +0.2 65.3 1 G049.205−00.343; W51
G49.369−0.302 19 23 11.204 14 26 37.06 1.5 3.2 1 +0.5 50.9, 62.9 1, 1 G049.384−00.298; W51
G49.459−0.353 19 23 32.908 14 29 55.71 1.9 3.9 1 +1.3 62.0, 68.6 1, 1 G049.490−00.381; W51
G49.488−0.380 19 23 42.119 14 30 41.99 4.0 11.1 1 +1.3 65.9 1 G049.490−00.381; W51
G52.753+0.334 19 27 32.385 17 43 27.32 0.3 0.3 1 +0.1 12.1, 45.2 1, 0 G052.757+00.334
G60.882−0.132 19 46 20.621 24 35 17.59 0.2 0.3 1 +0.0 22.3 1 G060.883−00.133; S87
G61.475+0.092 19 46 48.189 25 12 47.06 2.1 3.5 1 +0.5 (5.9), 21.1 (0), 1 G061.477+00.094; S88

Notes. The source name is constructed from the Galactic coordinates at which the peak of the continuum emission measured at 20′′ resolution occurs. The columns Fc denotes the flux density at the given coordinates for an angular resolution of 20′′ and 46′′. The column “Ext.” denotes whether the source is resolved (1 for resolved, 0 for unresolved sources), and the column α is the L-band spectral index, defined as I(ν) ∝ να, which are both taken from Bihr et al. (2016) and Wang et al. (2018). The central velocities of detected OH main line absorption are summarized in Col. 8 “OH velocities” (tentative, 3σ components are listed in brackets in Cols. 8 and 9). Association in position and velocity with an H II region is indicated with 1 in Col. 9. Criteria for the association are a smaller angular separation from the H II region than its radius, and a velocity difference of less than 10 km s −1. The name of the H II regions are obtained from the WISE catalog of H II-regions (Anderson et al. 2014). (*)Used 20′′ resolution data only in order not to blend OH absorption with adjacent maser.

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