Table 4: IRAS and 2MASS parameters. The two parts of the table give out the detected and un-detected sources respectively.

Source Name

$T_{\rm d}$(K) $\rm log[25/12]$ $\log[60/12]$ $L_{\rm bol}$($L_{\odot}$) 2MASS name J J-H H-K

02485+6902

39.51 1.03 1.79 1.3E+02 02530631+6914366 16.120 1.882 1.944
03035+5819 42.71 1.11 1.53 5.8E+04 03072452+5830433 12.757 1.876 1.361
06306+0437 31.27 0.60 1.47 9.4E+02 06331621+0434530 16.383 1.463 2.060
06501+0143 34.53 0.71 1.64 8.7E+03 06524617+0140190 16.337 1.259 1.701
18196-1331 43.37 0.57 1.49 6.6E+04 18222658-1330157 13.986 3.098 2.341
18265+0028m 30.20 1.21 2.01 7.4E+01 18290669+0030312 17.589 1.831 0.904
18308-0503 35.51 0.76 1.38 2.2E+04 18333054-0501020 14.529 1.731 2.815
18352-0148 29.17 0.53 1.65 5.6E+03 18375052-0145444 12.614 1.235 0.741
18361-0627 27.40 1.10 1.63 5.4E+04 18385227-0625141 14.644 1.501 0.639
18414-0339 28.47 0.60 1.79 2.9E+04 18440642-0336348 12.495 2.401 1.099
19363+2018 35.55 0.63 1.59 7.2E+03 19383146+2025220 15.080 1.419 2.125
19471+2641 25.21 0.58 1.57 9.2E+03 19490938+2649082 16.195 0.734 1.426
19474+2637 29.21 0.55 1.34 9.7E+03 19493223+2645264 15.186 0.618 1.088
20215+3725m 31.56 0.61 1.79 3.7E+02 20232729+3734539 16.982 2.094 3.058
23139+5939 35.97 1.23 2.09 2.0E+04 23161002+5955312 17.594 2.140 1.227
23151+5912 49.48 0.60 1.34 9.0E+04 23172102+5928480 14.104 2.832 1.712
18355-0650$^\circ$ 29.733 0.93 1.27 7.4E+05 18381218-0647413 14.51 1.21 0.74
20160+3911$^\circ$ 30.90 0.67 1.78 2.5E+04 20175373+3920452 11.88 1.39 0.67
          20174748+3920524 16.18 0.99 0.57

01133+6434

50.74 1.05 1.48 3.7E+02 01163754+6450408 13.947 0.822 0.736
06001+3014 38.06 0.33 1.58 4.4E+02 06032391+3014112 13.161 1.310 0.424
06446+0029 43.21 1.07 1.75 6.4E+02 06471336+0026065 14.302 2.323 2.000
07207-1435 42.80 1.24 2.20 4.6E+02 07230189-1441382 13.339 1.430 1.333
07427-2400 43.07 1.49 2.50 1.4E+03 07445196-2407399 15.857 2.032 2.497
18061-1927 27.68 0.70 1.60 1.0E+03 18090717-1927327 13.724 2.448 1.027
18403-0440 35.95 0.49 1.59 3.7E+02 18430155-0437010 14.834 0.865 1.164
19303+1651 38.19 0.64 1.77 2.0E+02 19323229+1657340 13.012 2.364 1.094
19560+3135 40.72 0.90 1.63 2.9E+02 19580326+3144068 14.909 1.736 1.091
20110+3321 37.82 0.68 1.28 9.6E+02 20130258+3330079 14.451 1.682 0.838
20144+3726 32.53 0.72 1.44 2.4E+02 20161456+3735295 13.802 1.072 0.740
20306+3749 37.38 0.57 1.78 4.8E+02 20323519+3759243 16.612 0.690 1.010
21008+4700 32.81 0.56 1.68 2.7E+02 21023019+4712232 14.351 1.774 0.664
21144+5430 42.87 1.09 1.80 2.0E+02 21155563+5443310 15.488 1.105 0.700
21334+5039 43.33 1.02 1.86 9.4E+02 21350991+5053048 15.093 0.618 2.285
21379+5106 37.98 1.07 2.13 1.5E+02 21394014+5120327 16.152 0.820 1.655
21391+5026 35.24 0.74 1.56 1.7E+02 21405742+5039583 15.244 1.556 0.781
21413+5442 44.44 0.74 1.40 3.2E+03 21430143+5456183 14.407 1.227 3.140
23004+5642 33.73 0.77 1.55 2.5E+02 23023471+5659170 16.206 1.004 0.558
05327-0457$^\circ$ 34.02 0.42 2.00 4.9E+03 05351438-0455226 12.856 0.765 0.600
20144+3526$^\circ$ 51.34 0.86 1.25 1.4E+03 20162196+3536062 13.943 2.473 1.903

Note: m Indicates the NH3 emission region has a minor peak; $\hbox{$^\circ$ }$ denotes the sources associated
with HII region and not included in the analysis.


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