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Table 2

Observed and derived parameters of dense cores.

ID α(J2000)a δ(J2000)a FWHMa PA Fluxa R TNH3a σNH3, tot Massa nH2 Σ Mvir α
(hh:mm:ss) (dd:mm:ss) (″ × ″) (deg) (mJy) (103AU) (K) (km s-1) (M) (107 cm-3) (g cm-2) (M)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13) (14)
Hub

c1 18:33:33.27 -8:39:16.0 1.58×1.17 127 20.1±2.0 2.9±0.3 19.8±0.6 0.84±0.03 9.43.4+5.2$^{+5.2}_{-3.4}$ 1.20.5+0.9$^{+0.9}_{-0.5}$ 3.21.2+2.0$^{+2.0}_{-1.2}$ 10.7±1.3 1.10.4+0.7$^{+0.7}_{-0.4}$
c2 18:33:33.18 -8:39:17.0 1.04×0.76 74 3.7±0.4 1.6±0.2 16.8±0.7 0.81±0.03 2.10.7+1.2$^{+1.2}_{-0.7}$ 1.50.6+1.1$^{+1.1}_{-0.6}$ 2.30.8+1.5$^{+1.5}_{-0.8}$ 5.7±0.7 2.71.0+1.5$^{+1.5}_{-1.0}$
c3 18:33:33.16 -8:39:15.0 0.96×0.64 84 90.7±9.0 1.3±0.1 21.7±0.9 1.09±0.04 37.613.3+20.8$^{+20.8}_{-13.3}$ 50.220.8+38.4$^{+38.4}_{-20.8}$ 61.623.8+40.0$^{+40.0}_{-23.8}$ 8.5±1.1 0.20.10+0.13$^{+0.13}_{-0.10}$
c4 18:33:33.14 -8:39:13.0 1.07×0.84 130 5.5±0.6 1.8±0.2 19.2±0.9 0.86±0.04 2.70.9+1.5$^{+1.5}_{-0.9}$ 1.40.6+1.1$^{+1.1}_{-0.6}$ 2.30.9+1.5$^{+1.5}_{-0.9}$ 7.0±1.0 2.61.0+1.0$^{+1.0}_{-1.0}$
c5 18:33:33.07 -8:39:15.0 0.88×0.82 58 6.9±0.7 1.5±0.2 21.1±1.0 1.04±0.04 3.01.0+1.6$^{+1.6}_{-1.0}$ 2.61.1+1.9$^{+1.9}_{-1.1}$ 3.71.4+2.3$^{+2.3}_{-1.4}$ 8.8±1.1 3.01.1+1.7$^{+1.7}_{-1.1}$
c6 18:33:33.05 -8:39:18.0 1.33×0.86 99 2.5±0.3 2.1±0.2 19.0±1.5 0.81±0.06 1.20.4+0.7$^{+0.7}_{-0.4}$ 0.40.2+0.3$^{+0.3}_{-0.2}$ 0.80.3+0.5$^{+0.5}_{-0.3}$ 7.4±1.4 6.03.6+2.4$^{+2.4}_{-3.6}$
c7 18:33:32.93 -8:39:17.0 0.99×0.81 103 2.8±0.3 1.6±0.2 24.4±1.8 0.64±0.04 1.00.4+0.6$^{+0.6}_{-0.4}$ 0.70.3+0.5$^{+0.5}_{-0.3}$ 1.10.4+0.7$^{+0.7}_{-0.4}$ 3.4±0.6 3.41.3+2.0$^{+2.0}_{-1.3}$
c8 18:33:32.82 -8:39:17.0 1.10×0.86 89 3.0±0.3 1.9±0.2 19.0±1.3 0.50±0.03 1.50.5+0.9$^{+0.9}_{-0.5}$ 0.70.3+0.5$^{+0.5}_{-0.3}$ 1.20.4+0.8$^{+0.8}_{-0.4}$ 2.2±0.4 1.50.6+0.9$^{+0.9}_{-0.6}$
c9 18:33:32.70 -8:39:14.0 2.79×2.02 128 9.8±0.1 5.3±0.5 16.5±0.7 0.64±0.03 5.92.1+3.1$^{+3.1}_{-2.1}$ 0.10.05+0.1$^{+0.1}_{-0.05}$ 0.60.2+0.4$^{+0.4}_{-0.2}$ 11±1.6 1.91.1+0.5$^{+0.5}_{-1.1}$

F1

c10 18:33:33.47 -8:38:46.0 0.74×0.64 90 9.9±0.1 1.0±0.1 17.0* 0.48*±0.03 5.82.1+3.1$^{+3.1}_{-2.1}$ 17.67.5+13.3$^{+13.3}_{-7.5}$ 17.06.4+10.5$^{+10.5}_{-6.4}$ 1.3±0.2 0.20.08+0.14$^{+0.14}_{-0.08}$
c11 18:33:33.26 -8:38:54.0 1.17×1.00 100 4.8±0.5 2.2±0.2 10.9±0.4 0.29±0.02 5.31.9+3.0$^{+3.0}_{-1.9}$ 1.60.6+1.2$^{+1.2}_{-0.6}$ 3.21.2+2.1$^{+2.1}_{-1.2}$ 0.5±0.04 0.10.03+0.05$^{+0.05}_{-0.03}$
c12 18:33:33.10 -8:38:59.0 1.24×1.21 177 11.3±0.1 2.5±0.3 12.0±0.4 0.46±0.03 10.73.9+6.3$^{+6.3}_{-3.9}$ 2.00.8+1.4$^{+1.4}_{-0.8}$ 4.71.8+3.0$^{+3.0}_{-1.8}$ 2.4±0.5 0.20.1+0.14$^{+0.14}_{-0.1}$
c13 18:33:32.98 -8:39:06.0 1.03×0.98 7 2.8±0.3 2.0±0.2 12.9±0.6 0.59±0.04 2.40.9+1.3$^{+1.3}_{-0.9}$ 1.00.4+0.7$^{+0.7}_{-0.4}$ 1.80.7+1.1$^{+1.1}_{-0.7}$ 3.4±0.36 1.40.6+0.9$^{+0.9}_{-0.6}$
c14 18:33:32.97 -8:39:08.0 1.67×1.49 95 4.4±0.4 3.4±0.3 15.3±0.9 0.45±0.03 2.91.0+1.7$^{+1.7}_{-1.0}$ 0.20.1+0.2$^{+0.2}_{-0.1}$ 0.70.3+0.5$^{+0.5}_{-0.3}$ 3.1±0.6 1.10.4+0.7$^{+0.7}_{-0.4}$
c15 18:33:32.95 -8:39:04.0 1.59×1.33 31 16.1±1.6 3.1±0.3 13.2±0.4 0.55±0.03 13.24.8+8.1$^{+8.1}_{-4.8}$ 1.30.5+1.0$^{+1.0}_{-0.5}$ 3.91.5+2.5$^{+2.5}_{-1.5}$ 4.6±0.7 0.40.14+0.22$^{+0.22}_{-0.14}$

F2

c16 18:33:32.52 -8:39:09.0 0.91×0.72 97 6.1±0.6 1.4±0.1 23.0±1.6 0.70±0.04 2.40.8+1.3$^{+1.3}_{-0.8}$ 2.61.1+2.0$^{+2.0}_{-1.1}$ 3.41.3+2.2$^{+2.2}_{-1.3}$ 3.5±0.5 1.50.6+0.9$^{+0.9}_{-0.6}$
c17 18:33:32.39 -8:39:09.0 0.94×0.69 103 6.0±0.6 1.4±0.1 18.7±1.1 0.40±0.02 3.01.1+1.7$^{+1.7}_{-1.1}$ 3.51.4+2.5$^{+2.5}_{-1.4}$ 4.51.7+2.9$^{+2.9}_{-1.7}$ 0.9±0.1 0.30.1+0.1$^{+0.1}_{-0.1}$
c18 18:33:31.56 -8:39:01.0 0.96×0.76 91 1.3±0.1 1.5±0.2 12.2±1.0 0.49±0.03 1.20.5+0.7$^{+0.7}_{-0.5}$ 1.00.4+0.7$^{+0.7}_{-0.4}$ 1.50.6+0.9$^{+0.9}_{-0.6}$ 1.7±0.4 1.40.5+0.4$^{+0.4}_{-0.5}$

Notes. The ★ symbol in Col. 1 indicates the protostellar core, while the name without a symbol pinpoints the prestellar core. a: taken from Cheng et al. (2024). The deconvolved radius, R, is derived from the equation Reff2(1/4ln2)Bmaj×Bmin,$\sqrt{R^2_{\rm{eff}}-(1/4\ln{2})\rm{Bmaj}\times \rm{Bmin}}$ where Reff=FWHMmaj×FWHMmin/2$R_{\rm{eff}}=\sqrt{\rm{FWHM_{\rm{maj}}} \times \rm{FWHM_{\rm{min}}}}/2$, Bmaj and Bmin represent the synthesized beam sizes. The uncertainty in flux is assumed to be 10%. The * symbol indicates that the median of the parameter for those cores with measurements is taken for that source. Uncertainties for Columns 8-10 and 12 were calculated using Monte Carlo methods. Uncertainties for Columns 5-7 and 11 were calculated through error propagation methods.

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