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Table C.1

Derived properties for the CAFFEINE clouds

Clumps YSOs
Cloud N22.15(a) N22.90(a) SFR22.15(b) SFR22.90 (b) SFE22.15 SFE22.90 N22.15(c) N22.90(c) SFR22.15(d) SFR22.90 (d) SFE22.15 SFE22.90
M⊙ Myr−1 M⊙ Myr−1 ×10−8Myr−1 ×10−8Myr−1 M⊙ Myr−1 M⊙ Myr−1 ×10−8Myr−1 ×10−8Myr−1
MonR2 15 4 20 9 2.06 6.19 98 7 105 13 10.86 8.71
R5180 6 3 159 98 2.45 2.3 5 0 106 - 1.64 -
NGC2264 6 4 34 28 1.75 6.87 50 6 62 32 3.16 7.59
GAL316 19 7 1152 - 10.71 - 30 5 84 89 0.78 3.06
114453 6 1 266 - 11.25 - 4 0 - - - -
SDC3l7p7 6 1 323 - 7.39 - 8 1 276 - 6.32 -
SDC3l7p9 10 3 304 - 11.54 - 23 10 102 57 3.87 8.53
RCW87 16 1 595 - 9.16 - 22 0 50 - 0.77 -
G322 3 2 - - - - 3 0 - - - -
SDC326 71 19 3700 - 6.5 - 91 18 574 190 1.01 1.16
G327 11 3 446 179 2.23 1.82 14 2 187 - 0.94 -
I15541 15 6 760 344 3.43 4.24 40 5 249 141 1.12 1.74
GAL332 14 3 577 207 3.56 5.55 24 3 186 - 1.15 -
G332 22 2 865 - 8.14 - 32 1 178 - 1.67 -
RCW106 38 4 2136 - 3.35 - 64 2 456 - 0.72 -
G333 5 1 236 - 7.38 - 6 0 266 - 8.33 -
G333.2 36 10 3032 726 4.23 2.75 28 4 271 - 0.38 -
I16175 4 1 148 - 2.51 - 6 2 273 - 4.6 -
G337.l 6 0 54 - 5.09 - 18 0 338 - 31.91 -
116351 4 1 83 49 1.8 4.42 17 0 246 - 5.35 -
116367 6 1 - - - - 21 5 233 72 7.14 17.36
SDC338 30 9 930 414 4.42 9.76 62 9 922 142 4.38 3.34
G337.9 11 1 683 - 5.88 - 22 2 356 - 3.07 -
G339 8 2 286 - 9.95 - 24 4 251 - 8.71 -
G340.8 6 2 284 - 3.2 - 13 2 103 - 1.17 -
OH34l 16 5 1144 398 7.04 9.68 33 7 256 178 1.57 4.34
SDC340 15 7 370 - 7.1 - 40 9 76 105 1.46 7.74
G341.9 2 2 370 - 4.24 - 4 0 - - - -
RCW116B 14 5 550 - 9.07 - 26 5 291 290 4.81 17.59
116572 12 3 266 - 7.95 - 31 6 142 101 4.24 21.54
SDC344 13 6 409 224 1.43 4.46 80 15 293 36 1.03 0.72
SDC345.4 5 2 195 - 3.57 - 14 2 48 - 0.88 -
SDC345.0 10 2 424 - 3.28 - 66 7 226 26 1.75 2.29
SDC348 34 16 1891 - 9.75 - 54 20 141 179 0.73 2.66
NGC6334N 8 3 162 - 2.04 - 24 1 94 - 1.18 -
I17233a 4 3 61 - 8.93 - 12 7 99 161 14.48 61.92
I17233b 8 0 246 - 9.71 - 1 0 - - - -
NGC6357SE 14 3 376 - 6.86 - 13 1 95 - 1.74 -
OH353 10 5 1671 - 6.57 - 33 4 114 - 0.45 -
G358.5 17 6 760 - 8.84 - 31 2 396 - 4.6 -
G005 15 2 - - - - 14 0 172 - 3.58 -
G008 11 3 470 - 7.05 - 5 0 108 - 1.62 -
SDC010 40 12 768 367 3.58 8.51 45 9 190 71 0.89 1.65
G010 8 0 357 - 1.79 - 16 1 225 - 1.13 -
W33 35 17 1671 905 1.07 2.84 142 18 513 258 0.33 0.81
SDC014 22 4 708 - 4.82 - 82 13 237 83 1.61 3.97
W42 5 0 267 - 2.58 - 5 1 1827 - 17.68 -
GO34 19 4 1193 474 1.24 3.34 65 5 645 476 0.67 3.35
W48B 11 4 323 240 2.8 6.21 40 5 314 262 2.72 6.79

Notes. (a)Numbers of protostellar clumps identified within contours of NH2=1022.15${N_{{{\rm{H}}_2}}} = {10^{22.15}}$ cm−2 and NH2=1022.90${N_{{{\rm{H}}_2}}} = {10^{22.90}}$ cm−2, respectively. (b)SFRs within the same contours derived from protostellar clumps using the method described in Sect. 4.2.2. (c)Numbers of Class I and II YSOs identified within contours of NH2=1022.15${N_{{{\rm{H}}_2}}} = {10^{22.15}}$ cm−2 and NH2=1022.90${N_{{{\rm{H}}_2}}} = {10^{22.90}}$ cm−2, respectively. (b)SFRs within the same contours derived from YSOs using the method described in Sect. 4.2.1.

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