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Table 3

Physical parameters of fragments.

Fragment Flux(a) Reff (b) θoutflow (c) θgradient (d) vLSR (e) Tgas (e) Mgas M* (f) Q
(mJy) (au) (°) (°) (km s−1) (K) (M) (M)
N30 e1 (VLA 3) 172.5 455 120 55.4 ± 7.0 8.48 ± 0.05 254 ± 13 0.44 ± 0.023 9.4 ± 1.8 5.2 ± 0.6
N30 e2 (VLA 1) 177.6 821 28/65 (*) –157.7 ± 1.0 8.62 ± 0.02 114±3 1.05 ± 0.031
N30 e5 (VLA 2) 37.3 253 55 11.54 ± 0.03 149 ± 7 0.17 ± 0.009
N56 e2 40.1 343 50 –24.8 ± 4.5 21.35 ± 0.17 168 ± 18 0.17 ± 0.019
N63 e1 649.9 621 60(*)/100/120/140 (*)/170 (*) 132.8 ± 2.4 −5.20 ± 0.05 137±11 3.17 ± 0.298
N68 e1 21.0 319 90 –6.91 ± 0.17 173 ± 39 0.08 ± 0.018
NW14 e1 108.3 602 115 3.7 ± 2.1 5.26 ± 0.05 180±11 0.40 ± 0.025 4.0 ± 0.7 3.9 ± 0.4

Notes. (a)1.3 mm dust continuum flux density with the fragment after subtracting the contribution from free-free emission (see Section 4.3). (b)Effective radii of the fragments Reff=A/π!$R_{\mathrm{eff}}=\sqrt{A / \pi}$ (see Section 3.1). (c)Position angle for identified CO outflow axis. (*) indicates the orientation of the unipolar CO outflow associated with the fragment. (d)Position angle of velocity gradient (the direction of increasing velocity, measured east of north) detected in CH3CN (123 − 113) emission. “…” means no clear velocity gradients were detected. (e)Fitting results of CH3CN emission average over the region of identified fragments in Section 4.3. (f)The central enclosed mass by fitting the Keplerian profile to the PV diagram of CH3CN (123 − 113) using KeplerFit.

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