Table 1 Open in new tab Summary of the...

Population	Number	f_turb	σ_f
All	81	1.76	0.09
NGC 1333	37	2.05	0.12
IC 348	23	1.36	0.09
L1448	14	1.8	0.2
L1455	7	1.5	0.4
Starless	17	1.8	0.2
Protostars^a	33	1.89	0.12
Class 0	19	2.04	0.16
Class I	14	1.7	0.2

Population	Number	f_turb	σ_f
All	81	1.76	0.09
NGC 1333	37	2.05	0.12
IC 348	23	1.36	0.09
L1448	14	1.8	0.2
L1455	7	1.5	0.4
Starless	17	1.8	0.2
Protostars^a	33	1.89	0.12
Class 0	19	2.04	0.16
Class I	14	1.7	0.2

Table 1

Summary of the turbulent fractions, f_turb, derived from Gaussian fits to the C¹⁸O J = 3 → 2 line at the peak of every SCUBA clump identified with clfind (Curtis & Richer 2010). The results are broken into either different regions in Perseus or clump classifications (see Section 2.2). The quoted errors (σ) are errors on the mean (⁠ formula ⁠) not sample deviations.

Population	Number	f_turb	σ_f
All	81	1.76	0.09
NGC 1333	37	2.05	0.12
IC 348	23	1.36	0.09
L1448	14	1.8	0.2
L1455	7	1.5	0.4
Starless	17	1.8	0.2
Protostars^a	33	1.89	0.12
Class 0	19	2.04	0.16
Class I	14	1.7	0.2

Population	Number	f_turb	σ_f
All	81	1.76	0.09
NGC 1333	37	2.05	0.12
IC 348	23	1.36	0.09
L1448	14	1.8	0.2
L1455	7	1.5	0.4
Starless	17	1.8	0.2
Protostars^a	33	1.89	0.12
Class 0	19	2.04	0.16
Class I	14	1.7	0.2

^a The Class 0 and Class I populations combined.

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