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Table 3

Result of the DUSTY model fit.

(1) (2) (3) (4) (5)
IRAS τ9.7 μm log(fbol)a Lb
name ×103L ×10-5M yr-1

165823059 15.9 11.70 4.0 1.7
170303053 10.9 11.75 3.5 1.0
171073330c 6.2 11.64 4.5 1.0
171283528c 41.3 11.30 9.9 8.7
171513642c 23.4 11.25 11.1 6.0
171712955c 10.9 11.63 4.7 1.4
172073632 34.2 11.00 19.8 12.8
172512821 23.328.2 11.4411.80 7.23.1 1.73.4
172922727 15.9 11.05 17.7 5.7
173163523 15.9 11.08 16.5 7.6
173232424 28.2 11.67 4.2 2.7
173413529c 5.16.2 11.0511.30 17.79.9 2.13.4
173502413c 9.010.9 11.5011.95 6.32.2 0.71.7
173513429 13.2 11.30 9.9 2.4
173612358c 15.9 11.57 5.3 2.1
173672722 34.2 11.60 5.0 6.8
173673633 10.913.2 10.8011.15 31.414.0 4.79.3
173683515 28.2 11.56 5.5 3.6
173923020 41.3 11.01 19.4 11.3
174182713 50.050.0 10.6711.02 42.418.9 18.040.4
174282438 15.9 11.40 7.9 3.2
174952534 15.928.2 10.7011.00 39.619.8 11.114.0
175212938 41.350.0 11.6011.88 4.92.6 2.33.7
175453056 50.0 11.77 3.4 3.3
175453317 15.9 11.50 6.3 2.6
175833346 5.1 11.40 7.9 1.6
175843147 34.2 11.45 7.0 4.3
180193121c 28.2 11.71 3.9 2.5
180402726 34.234.2 11.3511.65 8.94.4 2.85.7
180402953c 19.323.3 11.3011.65 9.94.4 2.44.6
180912437 15.919.3 11.5011.85 6.32.8 1.22.3
180922347 50.0 11.19 12.8 10.6
180922508 19.3 11.35 8.9 4.0
181952804 15.9 11.55 5.6 1.9
182012549c 5.1 11.25 11.2 2.2

Notes.

(a)

fbol in Watt m-2;

(b)

luminosity estimated using the distance of 8.0 kpc to the Galactic centre.

(c)

vexp = 14 km s-1 was assumed. Otherwise vexp is derived from either OH or CO radio data.

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