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Table 1

Molecular line emission characteristics of WISE H II regions in NGC 6334.

WISE H II source Type l b R R(13CO) V(13CO) (†)Emission C (††)Cmax (‡)Nclump
(°) (°) (″) (″) (km s−1) profile
G350.240+00.654 C 350.240 0.655 670 498 −3.8 I,V2 – 0.78 1
G350.401+01.037 G 350.401 1.037 372 546 −8.3 I,S 0.95 0.96 5
G350.482+00.951 K 350.482 0.952 96 96 −9.6 I,S 0.81 0.88 1
G350.505+00.956 K 350.505 0.957 96 84 −10.0 I,V3 – – 1
G350.594+01.149 G 350.594 1.149 1413 1314 −6.6 I,S – 0.84 26
G350.617+00.984 G 350.617 0.984 574 474 −8.1 I,S 0.76 0.80 14
G350.675+00.832 G 350.675 0.832 108 156 −6.8 I,V3 – 0.79 1
G350.707+00.999 C 350.707 0.999 86 84 −5.0 I,S 0.76 0.89 1
G350.710+00.641 G 350.710 0.642 737 330 −4.2 I,S 0.85 0.98 21
G350.716+01.044 Q 350.716 1.045 50 −4.1 F 0.77 0.79
G350.871+00.763 Q 350.871 0.763 86 36 −1.9 I 0.82 0.83
G350.889+00.728 Q 350.889 0.729 76 96 −2.0 I,V2 – 0.83 1
G350.958+00.358 K 350.958 0.359 179 135 I,S – 0.92
G350.995+00.654 K 350.995 0.654 428 330 −3.3 I 0.90 0.92 22
G351.017+00.856 Q 351.017 0.857 59 I 0.80 0.80
G351.094+00.800 Q 351.094 0.800 116 −4.5 I,V2 – 0.79
G351.130+00.449 K 351.130 0.450 549 534 −5.1 I,S 0.95 0.96 8
G351.153+00.623 Q 351.153 0.623 68 −4.9 I 0.80 0.83 1
G351.170+00.704 K 351.170 0.704 171 300 −5.1 I,V3 – – 3
G351.246+00.673 K 351.246 0.673 131 108 −3.3 CP – – 4
G351.261+01.016 K 351.261 1.016 114 111 1.4 I,S 0.81 0.81 1
G351.311+00.663 K 351.311 0.663 119 162 −2.0 I,V2 – – 3
G351.348+00.593 G 351.348 0.593 125 54 −2.5 I,S 0.80 0.91 3
G351.360+01.015 K 351.360 1.015 129 66 1.3 I,V4 – –
G351.367+00.640 K 351.367 0.641 107 132 −2.9 I,S 0.83 0.95 4
G351.383+00.737 K 351.383 0.737 303 222 −3.6 I,S 0.81 0.98 14
G351.420+00.637 Q 351.420 0.638 52 −5.6 F – – 3
G351.424+00.650 G 351.424 0.651 99 −5.0 CP – – 4
G351.462+00.556 G 351.462 0.557 68 42 −3.6 I 0.84 0.88
G351.479+00.643 Q 351.479 0.644 68 −4.2 F – 0.76 2
G351.651+00.510 K 351.651 0.510 234 96 −1.7 I,V2 – 0.80
G351.676+00.610 G 351.676 0.611 130 162 −2.4 I 0.89 0.90
G351.693+00.671 K 351.693 0.672 175 180 −2.1 I,V2 – 0.79
G351.766+00.492 G 351.766 0.493 217 318 −1.1 CP – 0.91
G351.835+00.756 Q 351.835 0.757 87 −0.2 I 0.76 0.84
G351.922+00.638 Q 351.922 0.638 86 69 −0.3 I,S – 0.86 1
G352.060+00.636 Q 352.060 0.636 99 1.0 F 0.76 0.76
G352.132+00.663 C 352.132 0.663 143 72 0.8 I 0.80 0.81
G352.171+00.307 C 352.171 0.307 423 378 −1.9 I,S – 0.90 2
G352.486+00.799 C 352.486 0.799 43 −2.3 I,V4 – 0.83
G352.493+00.793 C 352.493 0.794 40 42 −2.4 CP – –
G352.529+00.775 Q 352.529 0.775 22 −1.7 I,V4 0.77 0.77

Notes. Columns 1 to 5 (H II region name, type, longitude, latitude, and radius, respectively) are taken from Anderson et al. 2014. The sizes of the molecular shells and rings (R(13CO)), molecular line velocities (V(13CO)), and contrast parameter values (C) are determined from this work. (†) 13CO radial profiles. CP: centrally peaked, I: increasing profile, S: shell-like feature, F: flat profile. V1: [−15, −10] km s−1, V2: [−10,−5] km s−1, V3: [−5,0] km s−1, V4: [0,+5] km s−1.(‡‡) Maximum value of the contrast in one of the velocity ranges.(‡) Number of ATLASGAL clumps (from Urquhart et al. 2018a) located at H II radii range 0.6R–1.2R.

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