Notes. ^(a) Dust temperature estimated by Cao et al. (2021). The 1-σ uncertainty of T is σ_T = 4 K. ^(b)Gasmass estimated by Cao etal. (2021). Monte-Carlo simulations show that the 1-σ uncertainty of M_gas is ~0.26 dex (~64%). ^(c)Orientation of the velocity gradient revealed by the selected line emission. ^(d)Detection of dense gas tracers, CH₃CN, Ch₃OH, and H₂CO, in each dust condensation associated with outflow. Information on the transitions of these molecules is listed in Table 2. means no dense gas tracers were detected as showing the kinematics. “C¹⁸O” means the C¹⁸O (2−1) emission in Field8 MM1 also traces dense gas surrounding the condensation and reveals the evidence of a rotating structure. ^(e)Radio sources identified by Wang et al. (2022). “UC/HC” means the radio detection is likely from the ultra- or hyper-compact HII region. “Jet/Wind” means the radio detection is likely from a radio jet or wind. “N” means no radio source coincides with the condensation. ^(f)IR Classification identified by Kryukova et al. (2014). “Class” implies the mid-infrared color of these condensations, which can in turn indicate the YSO evolutionary stage of these condensations. “FS” means a “flat spectrum” that has a spectral index, α, ranging from −0.3 to 0.3. The discussions of the mid-infrared colors are shown in Sect. 4.2.2. ^(g)Classifications of the condensations. “Outflow-associated” means these condensations are associated with outflow. “Dense-gas-traced” are condensations included in “outflow-associated” condensations that have emission of dense gas tracers. “Disk candidate” condensations are included in dense-gas-traced condensations showing evidence of a rotating disk. The classifications of the condensations are described in Sect. 3.2. ^(h)The clear velocity gradient from line emission away from a potential outflow central source. So, it is not identified as a disk candidate. ^(*)The sources are saturated or unresolved in a 24 μm image, which means photometry is unavailable.