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Table 2

Parameters of dense cores.

Index α(J2000) δ(J2000) FWHM PA R F1.3 mm int$F_{1.3 \mathrm{~mm}}^{\text {int }}$ T NH 3a$T_{\rm NH_3}^{\rm a}$ σtot Mcore nH2 Σ α
hh:mm:ss dd:mm:ss ′′×′′ deg 103 AU mJy K km s−1 M 106 cm−3 g cm−2
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13)
Fs
c1 19:09:53.33 +7:56:50.5 0.52×0.38 117 2.0±0.2 1.6±0.1 16.4* 0.35±0.01* 3.6-1.3+2.0$3.6_{-1.3}^{+2.0}$ 13.7-0.6+1.0$13.7_{-0.6}^{+1.0}$ 2.6-1.0+1.7$2.6_{-1.0}^{+1.7}$ 0.4-0.1+0.1$0.4_{-0.1}^{+0.1}$
c2 19:09:53.42 +7:57:03.4 0.66×0.50 87 2.6±0.3 1.1±0.1 21.0±0.6 0.39±0.01 1.7-0.6+0.9$1.7_{-0.6}^{+0.9}$ 3.0-0.1+0.2$3.0_{-0.1}^{+0.2}$ 0.7-0.3+0.5$0.7_{-0.3}^{+0.5}$ 1.3-0.1+0.4$1.3_{-0.1}^{+0.4}$
c3 19:09:53.42 +7:57:05.7 0.52×0.46 132 2.2±0.2 0.8±0.1 16.0±0.6 0.30±0.01 1.9-0.7+1.1$1.9_{-0.7}^{+1.1}$ 5.4-0.2+0.4$5.4_{-0.2}^{+0.4}$ 1.1-0.4+0.7$1.1_{-0.4}^{+0.7}$ 0.6-0.1+0.2$0.6_{-0.1}^{+0.2}$
c4✶ 19:09:53.55 +7:56:51.7 0.60×0.56 115 2.5±0.1 2.5±0.3 50* 0.48±0.01* 1.4-0.5+0.8$1.4_{-0.5}^{+0.8}$ 2.6-0.1+0.2$2.6_{-0.1}^{+0.2}$ 0.6-0.2+0.4$0.6_{-0.2}^{+0.4}$ 2.3-0.2+0.6$2.3_{-0.2}^{+0.6}$
c5✶ 19:09:53.61 +7:56:55.2 0.88×0.66 165 3.4±0.3 12.6±0.6 50.0*(16.5) 0.48±0.01* 7.3-2.6+4.1$7.3_{-2.6}^{+4.1}$ 5.7-0.2+0.4$5.7_{-0.2}^{+0.4}$ 1.8-0.7+1.1$1.8_{-0.7}^{+1.1}$ 0.6-0.2+0.2$0.6_{-0.2}^{+0.2}$
c6 19:09:53.71 +7:56:53.2 1.00×0.56 105 3.3±0.3 4.1±0.2 13.8±0.1 0.34±0.01* 11.8-4.2+6.4$11.8_{-4.2}^{+6.4}$ 9.7-0.4+0.7$9.7_{-0.4}^{+0.7}$ 3.0-1.1+1.9$3.0_{-1.1}^{+1.9}$ 0.2-0.1+0.1$0.2_{-0.1}^{+0.1}$
c7 19:09:53.91 +7:56:49.8 1.44×0.84 93 4.9±0.5 5.2±0.3 17.5±0.7 0.40±0.04 10.7-3.8+6.0$10.7_{-3.8}^{+6.0}$ 2.8-0.1+0.2$2.8_{-0.1}^{+0.2}$ 1.3-0.5+0.8$1.3_{-0.5}^{+0.8}$ 0.4-0.1+0.1$0.4_{-0.1}^{+0.1}$
c8✶ 19:09:53.92 +7:56:52.8 0.96×0.58 164 3.3±0.3 1.9±0.1 30*(13.7) 0.41±0.01* 2.0-0.7+1.1$2.0_{-0.7}^{+1.1}$ 1.6-0.1+0.1$1.6_{-0.1}^{+0.1}$ 0.5-0.2+0.3$0.5_{-0.2}^{+0.3}$ 1.6-0.3+0.5$1.6_{-0.3}^{+0.5}$
c9 19:09:53.96 +7:56:47.6 0.60×0.40 104 2.2±0.2 1.1±0.1 16.4* 0.30±0.01 2.4-0.9+1.3$2.4_{-0.9}^{+1.3}$ 6.9-0.3+0.5$6.9_{-0.3}^{+0.5}$ 1.4-0.5+0.9$1.4_{-0.5}^{+0.9}$ 0.5-0.1+0.2$0.5_{-0.1}^{+0.2}$
Fn
c10 19:09:53.29 + 7:57:10.6 1.16×0.68 60 4.0±0.4 7.9±0.4 13.7±2.7 0.24±0.02 22.9-9.0+17.5$22.9_{-9.0}^{+17.5}$ 11.2-0.5+1.4$11.2_{-0.5}^{+1.4}$ 4.1-1.7+3.7$4.1_{-1.7}^{+3.7}$ 0.1-0.1+0.1$0.1_{-0.1}^{+0.1}$
c11 19:09:53.39 +7:57:12.8 0.78×0.34 109 2.3±0.2 2.8±0.1 23.4±0.2 0.54±0.02 4.0-1.4+2.2$4.0_{-1.4}^{+2.2}$ 10.5-0.4+0.8$10.5_{-0.4}^{+0.8}$ 2.2-0.8+1.5$2.2_{-0.8}^{+1.5}$ 0.9-0.3+0.2$0.9_{-0.3}^{+0.2}$
c12 19:09:53.43 +7:57:09.2 1.00×0.62 179 3.5±0.4 1.8±0.1 17.3±0.5 0.28±0.01 3.8-1.4+2.1$3.8_{-1.4}^{+2.1}$ 2.7-0.1+0.2$2.7_{-0.1}^{+0.2}$ 0.9-0.3+0.6$0.9_{-0.3}^{+0.6}$ 0.4-0.1+0.2$0.4_{-0.1}^{+0.2}$
c13✶ 19:09:53.44 +7:57:15.4 0.56×0.28 170 1.8±0.2 3.9±0.2 30*(18.1) 0.65±0.01 4.1-1.5+2.2$4.1_{-1.5}^{+2.2}$ 21.2-0.9+1.6$21.2_{-0.9}^{+1.6}$ 3.6-1.3+2.2$3.6_{-1.3}^{+2.2}$ 1.1-0.2+0.2$1.1_{-0.2}^{+0.2}$
c14✶ 19:09:53.56 +7:57:15.4 0.9×0.72 135 3.6±0.4 19.4±1.0 100.0*(15.5) 0.75±0.01 5.3-1.9+2.9$5.3_{-1.9}^{+2.9}$ 3.5-0.1+0.3$3.5_{-0.1}^{+0.3}$ 1.2-0.4+0.7$1.2_{-0.4}^{+0.7}$ 2.1-0.8+0.5$2.1_{-0.8}^{+0.5}$
c15 19:09:53.73 +7:57:13.8 1.34×0.82 74 4.7±0.5 7.6±0.4 16.8* 0.43±0.01 16.6-6.1+9.2$16.6_{-6.1}^{+9.2}$ 5.1-0.2+0.4$5.1_{-0.2}^{+0.4}$ 2.2-0.8+1.4$2.2_{-0.8}^{+1.4}$ 0.3-0.2+0.1$0.3_{-0.2}^{+0.1}$
c16 19:09:53.75 +7:57:15.9 0.42×0.36 157 1.7±0.2 1.4±0.1 16.8* 0.34±0.01 2.9-1.0+1.6$2.9_{-1.0}^{+1.6}$ 16.9-0.7+1.2$16.9_{-0.7}^{+1.2}$ 2.8-1.1+1.8$2.8_{-1.1}^{+1.8}$ 0.4-0.1+0.1$0.4_{-0.1}^{+0.1}$
c17 19:09:53.96 +7:57:16.2 1.10×0.58 178 3.5±0.4 1.6±0.1 16.8* 0.41±0.03 3.6-1.3+1.9$3.6_{-1.3}^{+1.9}$ 2.5-0.1+0.2$2.5_{-0.1}^{+0.2}$ 0.8-0.3+0.5$0.8_{-0.3}^{+0.5}$ 1.0-0.1+0.2$1.0_{-0.1}^{+0.2}$
c18 19:09:54.37 + 7:57:22.2 0.78×0.44 152 2.6±0.3 2.5±0.1 11.0±0.9 0.24±0.01 10.2-3.8+5.9$10.2_{-3.8}^{+5.9}$ 16.7-0.7+1.3$16.7_{-0.7}^{+1.3}$ 4.1-1.6+2.8$4.1_{-1.6}^{+2.8}$ 0.1-0.1+0.1$0.1_{-0.1}^{+0.1}$
c19✶ 19:09:54.40 +7:57:24.1 0.90×0.80 179 3.9±0.2 3.9±0.4 50.0*(11.0) 0.44±0.01 2.2-0.8+1.2$2.2_{-0.8}^{+1.2}$ 1.2-0.1+0.1$1.2_{-0.1}^{+0.1}$ 0.4-0.2+0.3$0.4_{-0.2}^{+0.3}$ 1.9-0.3+0.5$1.9_{-0.3}^{+0.5}$
c20 19:09:54.46 +7:57:40.0 0.88×0.50 81 3.0±0.3 2.6±0.1 16.8* 0.37±0.01* 5.6-2.0+3.1$5.6_{-2.0}^{+3.1}$ 6.4-0.3+0.5$6.4_{-0.3}^{+0.5}$ 1.8-0.7+1.2$1.8_{-0.7}^{+1.2}$ 0.4-0.1+0.1$0.4_{-0.1}^{+0.1}$
c21 19:09:54.52 +7:57:38.4 0.98×0.46 148 3.0±0.3 2.2±0.1 16.8* 0.37±0.01* 4.8-1.7+2.6$4.8_{-1.7}^{+2.6}$ 5.4-0.2+0.4$5.4_{-0.2}^{+0.4}$ 1.5-0.6+1.0$1.5_{-0.6}^{+1.0}$ 0.5-0.1+0.1$0.5_{-0.1}^{+0.1}$
c22 19:09:54.53 +7:57:32.6 0.56×0.36 157 2.0±0.2 0.8±0.1 16.8* 0.37±0.01 1.7-0.6+0.9$1.7_{-0.6}^{+0.9}$ 6.4-0.3+0.5$6.4_{-0.3}^{+0.5}$ 1.2-0.5+0.8$1.2_{-0.5}^{+0.8}$ 0.9-0.1+0.1$0.9_{-0.1}^{+0.1}$
c23 19:09:54.55 +7:57:27.0 0.88×0.50 148 3.0±0.3 1.5±0.1 21.5±1.0 0.49±0.01 2.4-0.9+1.3$2.4_{-0.9}^{+1.3}$ 2.9-0.1+0.2$2.9_{-0.1}^{+0.2}$ 0.8-0.3+0.5$0.8_{-0.3}^{+0.5}$ 1.7-0.2+0.4$1.7_{-0.2}^{+0.4}$
c24 19:09:54.55 +7:57:34.2 0.66×0.26 123 1.9±0.2 0.4±0.1 16.8* 0.37±0.01 1.0-0.3+0.5$1.0_{-0.3}^{+0.5}$ 4.6-0.2+0.3$4.6_{-0.2}^{+0.3}$ 0.8-0.3+0.5$0.8_{-0.3}^{+0.5}$ 1.5-0.1+0.2$1.5_{-0.1}^{+0.2}$
c25 19:09:54.61 +7:57:23.8 1.22×0.70 139 4.1±0.4 3.6±0.2 19.8±0.4 0.41±0.01 6.4-2.3+3.4$6.4_{-2.3}^{+3.4}$ 2.8-0.1+0.2$2.8_{-0.1}^{+0.2}$ 1.1-0.4+0.7$1.1_{-0.4}^{+0.7}$ 0.6-0.2+0.1$0.6_{-0.2}^{+0.1}$
c26 19:09:54.71 +7:57:30.4 0.52×0.44 61 2.2±0.2 0.9±0.1 16.8* 0.37±0.01 1.9-0.7+1.0$1.9_{-0.7}^{+1.0}$ 6.0-0.2+0.4$6.0_{-0.2}^{+0.4}$ 1.2-0.5+0.8$1.2_{-0.5}^{+0.8}$ 0.8-0.1+0.1$0.8_{-0.1}^{+0.1}$

Notes. The * symbol indicates the protostellar core while the name without a symbol pinpoints the candidate prestellar core. The uncertainty in flux is assumed to be 5%. a: temperature given in Lu et al. (2018); the c14 core associated with a UC H II region corresponds to an assumed temperature of 100 K, the protostellar cores with outflows to 50 K, and the protestellar cores without outflows to 30 K. For cores without measurements we replace them with the average of the other cores in the same region and mark them with *. Uncertainties for columns 10-13 were calculated using Monte Carlo methods. Uncertainties for columns 6-9 were calculated through error propagation method.

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