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Table 4

Derived column density and abundances, and physical parameters of associated dust clumps.

Source NSiO (cm−2) XSiO Dist. (kpc) Tdust (K) Log(Lbol) (L) Log(Mclump) (M)
G018.82−00.28MM1 1.06×1013 23.055 22.936 9.34×10−11 12.6 18.7 4.806 4.369 1.34×10−3 9.71×10−5
G019.27+00.07MM2 7.44×1013 22.714 22.560 1.44×10−10 2.8 12.1 2.079 2.713 2.31 ×10−6
G022.35+00.41MM1 1.30×1013 22.953 22.465 1.45×10−10 3.6 13.1 2.420 3.057 6.70×10−6 4.23×10−6
G023.60+00.00MM1 5.97×1012 22.930 22.771 7.02×10−11 5.9 16.9 3.782 3.519 1.21×10−6 2.42×10−5
G023.60+00.00MM2 8.89×1012 22.806 22.673 1.39×10−10 3.6 16.7 3.362 3.064 1.24×10−5
G31.41 + 0.31 5.57×1012 23.696 1.12×10−11 4.9 22.0 4.800 3.852 1.52×10−4 1.30×10−5
G33.92+0.11 4.49×1012 23.048 22.857 4.02×10−11 6.9 27.4 5.226 3.726 7.73×10−7 5.26×10−6
G34.26+0.15 2.87×1013 23.917 23.253 3.48×10−11 2.9 29.2 5.330 3.776 3.34×10−4 2.58×10−5
G45.47+0.05 1.06×1013 22.915 22.763 1.29×10−10 7.7 29.0 5.557 3.779 2.61 ×10−5
HM18507+0121 3.40×1013 23.249 22.679 1.92×10−10 2.9 20.5 4.042 3.260 1.37×10−4 2.25×10−5
HM18517+0437 3.50×1012 1.9 1.50×10−6 7.47×10−7
HM18530+0215 7.74×1012 22.855 22.624 1.08×10−10 4.7 26.1 4.674 3.283 6.20×10−6
HM18566+0408 8.28×1012 22.908 22.606 1.02×10−10 4.9 22.5 4.365 3.293 9.69×10−6 4.64×10−6
HM19217+1651 5.22×1012 22.659 22.373 1.15×10−10 10.9 29.1 5.035 3.457 2.37×10−4 4.04×10−5

Notes. Only a fraction of the entire table is presented here, and the full table is available at CDS. The properties of dust clumps are taken from the ATLASGAL point source catalog (Urquhart et al. 2018, 2022). N(H2) preceded by superscript a is from the ATLASGAL catalog, and the other one marked by b is measured from the Hi-GAL PPMAP over the observed KVN beam size. The listed X(SiO) are determined using N(H2) from the ATLASGAL catalog. All other clump physical parameters (i.e., Tdust, Log(Lbol), and Log(Mclump)), and distance also come from the ATLASGAL catalog. and are recalculated with the distance from the point source catalog and velocity-integrated intensities of H2O and Class I CH3OH are taken from Kim (2016) and Kim et al. (2019).

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