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Table A.4:

Deconvolved C18O(2-1) clump diameter, Galactocentric distance and various mass estimates.

Source 		D $R_{\rm gal}$ $T_{\rm dust}$ $M_{\rm clump}$( $T_{\rm dust}$) $M_{\rm clump}$(T = 15-60 K) $M_{\rm vir}$ $M_{\rm dust}$ $V_{{\rm rot}}$ $M_{\rm rot}$
  (pc) (kpc) (K) ($M_{\odot}$) ($M_{\odot}$) ($M_{\odot}$) ($M_{\odot}$) (km s-1) ($M_{\odot}$)
05358+3543a 0.44 10.3 47 129 86-153 815 127 -- --
G213.61-12.6 0.45 10.3 20 196 192-345 344 1800 -- --
G189.78+0.34 0.24 10.3 20 55 53-96 227 150 -- --
G192.58-0.04 0.26 11.1 20 94 92-164 230 500 -- --
G192.60-0.05 0.31 11.1 20 138 135-241 354 460 -- --
18151-1208_2a 0.63 5.7 18.5d 173 172-306 810 475 -- --
18151-1208_3 0.52 5.7 47 129 86-153 107 53 0.49 14
18151-1208_1 0.52 5.7 47 250 165-297 595 211 0.56e 15e
G18.15-0.28 0.42 6.1 20 236 231-414 452 280 1.05c 44c
G18.18-0.30 0.34 6.1 20 125 123-219 321 110 0.27 2.2
18223-1243 0.45 5.1 21 202 197-350 425 980 -- --
18228-1312 0.64 5.7 34 542 438-779 1185 740 0.51c 15c
G19.27+0.1M2a 0.44 6.3 15 50 50-90 244 114 -- --
G19.27+0.1M1a 0.35 6.3 15 20 20-35 106 113 -- --
18236-1205 0.36 6.2 26 135 124-220 412 780 0.49 9.4
18264-1152 0.43 3.5 27 121 108-194 434 1100 0.45e 14e
G23.60+0.0M1 0.76 3.8 15 305 305-545 690 580 0.40 12.4
18316-0602 0.44 5.9 30 250 216-383 1064 1000 0.62 25
G23.60+0.0M2 0.53 5.2 15 73 73-130 468 233 -- --
18317-0513 0.43 5.8 31 153 130-230 239 770 0.45 9.6
G24.08+0.0M2a 0.42 5.3 15 21 21-38 159 201 -- --
G24.33+0.1M1 0.57 3.7 15 132 132-235 412 5470 -- --
G24.33+0.1M4 0.65 3.7 15 145 145-257 1175 1390 -- --
G24.33+0.1M2a 0.65 3.6 15 85 85-151 515 417 -- --
G24.60+0.1M2a 0.80 3.7 15 115 115-206 618 1630 0.30e 9.2e
G24.60+0.1M1 0.79 5.4 15 133 133-237 650 192 0.47 20
G25.04-0.2M1 0.93 5.0 15 305 305-543 376 441 0.29e 5.2e
G25.04-0.2M4b --b 5.6 15 --b --b 341 491 -- --
G25.04-0.2M2a 0.91 5.0 15 111 111-198 472 166 -- --
G28.28-0.35 0.69 6.2 20 330 324-578 939 650 0.83c 41c
18507+0121 0.64 3.7 28 390 345-614 2419 2000 0.62 19
G34.43+0.2M1a 0.42 5.8 15 73 73-131 1016 1187 0.33 5.5
G34.43+0.2M3a 0.26 5.8 15 73 73-131 144 301 -- --
G34.24+0.13 0.75 5.9 20 737 725-1290 532 140 -- --
18517+0437 0.61 6.4 38 346 262-468 467 504 0.70e 35e
G34.77-0.6M2a 0.70 6.3 15 87 87-155 2825 188 -- --
G35.39-0.3M4a 0.78 6.4 15 95 95-169 138 108 -- --
G38.95-0.5M1 0.69 6.6 15 223 223-398 696 117 -- --
19035+0641 0.24 7.0 51 49 32-55 819 185 0.41e 4.5e
19095+0930 0.33 6.5 34 240 193-345 1166 500 0.67 22
20216+4107 0.30 8.3 46 57 40-69 71 31 0.35 4.0
20332+4124 0.86 8.8 56 789 465-829 813 286 0.83 52
22134+5834 0.46 9.5 61 228 126-226 255 83 -- --
22570+5911_2b --b 11.3 54 --b --b 957 131 -- --
22570+5912_1 0.86 11.3 54 646 289-696 564 305 0.42 18
23033+5951 0.59 10.2 52 410 254-454 595 250 -- --
23139+5939 0.65 11.2 41 418 304-459 934 404 0.30 4.9
23151+5912 0.54 11.8 68 574 291-523 581 282 0.34 5.3

Notes. (a) Bad quality C18O maps: $M_{\rm clump}$ and D estimates not reliable; (b) C18O(2-1) map not shown in Fig. B.1: no C18O(2-1) quantities derived (see text); (c) C18O velocity gradient likely due to multiple components; (d) dust temperature from Sridharan et al. (2005); (e) C18O velocity gradient roughly aligned with outflow axis: it may be tracing the outflow.


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