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Table 4

Classification and physical parameters of HMSCs.

Name (1) Tdust (2) (3) Mclump Lclump LM rpc vlsr Distance (4) KDA (5) Association Morphology (6)
(K) (103 cm−3) (1021 cm−2) (M) (L) (L /M) (pc) (km s−1) (kpc)
G003.0371−0.0582 13.8 1.17(0.35) 53.6(8.0) 1.21(0.64) × 104 8.28(5.07) × 103 0.68(0.23) 3.3 85 13(3.3) NA C
G003.0928+0.1680 14.2 1.96(0.58) 80.2(12.0) 2.42(1.28) × 104 1.75(1.06) × 104 0.72(0.24) 3.5 150(0.12) 16(4.1) NA C
G003.1447+0.4733 14.3 1.90(0.29) 15.4(2.3) 9.17(1.39) × 102 7.16(2.70) × 102 0.78(0.29) 1.2 70(1.9) 11(0.12) NA F
G003.2110+0.6465 14.5 5.06(0.80) 22.9(3.4) 1.89(0.34) × 102 1.59(0.62) × 102 0.84(0.32) 0.51 18(0.25) 2.9(0.15) NA F
G003.2278+0.4924 14.4 6.14(0.97) 31.4(4.7) 2.34(0.43) × 102 1.88(0.72) × 102 0.8(0.29) 0.51 20(0.88) 2.9(0.15) IR DARK NA F
G003.2413+0.6334 13 19.2(8.1) 59.7(9.0) 4.99(4.03) × 102 2.15(1.83) × 102 0.43(0.14) 0.45 41 4(1.6) NA F
G003.2702+0.4446 13.8 6.02(0.95) 36.9(5.5) 3.87(0.70) × 102 2.34(0.85) × 102 0.6(0.21) 0.61 27 2.9(0.15) NA C
G004.4076+0.0993 18.1 123(19) 20.8(3.1) 8.99(1.63) × 101 3.60(1.71) × 102 4(1.9) 0.14 10(0.35) 2.9(0.15) AS S
G004.7473−0.7623 12.7 6.53(0.99) 71.0(10.7) 4.89(0.78) × 103 1.81(0.56) × 103 0.37(0.11) 1.4 210 9.4(0.24) NA I
G005.3876+0.1874 12.9 52.7(8.3) 38.3(5.7) 1.76(0.32) × 102 7.44(2.52) × 101 0.42(0.14) 0.23 11(0.74) 2.9(0.15) AS F
G005.8357−0.9958 15.4 6.59(1.05) 23.9(3.6) 1.25(0.23) × 102 1.50(0.62) × 102 1.2(0.48) 0.4 13 2.9(0.15) Z H PA I
G005.8523−0.2397 12.1 12.2(1.9) 45.0(6.7) 2.30(0.42) × 102 7.28(2.29) × 101 0.32(0.09) 0.4 17(0.13) 3(0.15) HISA NA I
G005.8799−0.3591 16.5 30.0(4.8) 51.2(7.7) 2.43(0.44) × 102 4.38(1.80) × 102 1.8(0.72) 0.3 5.8(0.1) 2.9(0.15) HISA AS S
G005.8893−0.4565 19.4 97.0(15.4) 46.6(7.0) 2.16(0.39) × 102 1.16(0.53) × 103 5.4(2.4) 0.2 9.7(0.23) 2.9(0.15) IR DARK AS S
G005.8917−0.3567 17 20.6(3.3) 35.4(5.3) 2.46(0.45) × 102 5.44(2.36) × 102 2.2(0.93) 0.35 5.8(0.13) 2.9(0.15) IR DARK AS S
G005.9394−0.3754 17.2 14.6(2.3) 21.0(3.2) 1.32(0.24) × 102 3.27(1.49) × 102 2.5(1.1) 0.31 6.1(0.1) 2.9(0.15) HISA AS S
G006.2130−0.5937 15.8 23.6(3.7) 34.9(5.2) 1.67(0.30) × 102 2.44(1.00) × 102 1.5(0.58) 0.29 18(0.11) 3(0.15) Z H AS F
G006.4609−0.3902 17.9 6.96(1.10) 4.58(0.69) 2.02(0.37) × 101 7.12(3.54) × 101 3.5(1.7) 0.22 19 3(0.15) NA I
G006.4916−0.3322 17.7 9.88(1.57) 4.54(0.68) 2.17(0.40) × 101 6.81(3.35) × 101 3.1(1.5) 0.2 2.2 2.9(0.15) NA I
G006.4982−0.3222 17.6 1.94(0.31) 8.96(1.34) 5.66(1.03) × 101 1.65(0.79) × 102 2.9(1.4) 0.46 5.1(0.25) 2.9(0.15) NA I

Notes. (1) Full table is available at the CDS. (2)The typical error of Tdust estimated by Y17 is about 2–3 K. (3)The typical error of estimated is about 15% from Y17. (4)The distance error is taken from the results of distance calculator and its typical value is less than 1 kpc. The distance errors are propagated to the calculation of other physical parameters. (5) We solve the KDA with several ways: IR DARK. IR extinction. H I SA. H I self-absorption. Z H. The scale height in the Galactic plane. TANGENT. The tangentline of sight. LITERAT. The literature in Urquhart et al. (2018). See Appendix A for more information. (6) The detailed explanation about the morphology is in Appendix B.

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