Äîêóìåíò âçÿò èç êýøà ïîèñêîâîé ìàøèíû. Àäðåñ îðèãèíàëüíîãî äîêóìåíòà : http://www.mrao.cam.ac.uk/~eic22/Papers/CR10b_suppmaterial.pdf Äàòà èçìåíåíèÿ: Mon Jul 26 21:36:58 2010 Äàòà èíäåêñèðîâàíèÿ: Tue Oct 2 07:50:13 2012 Êîäèðîâêà: Ïîèñêîâûå ñëîâà: âíåøíèå ïëàíåòû

Mon. Not. R. Astron. Soc. 000, 000­000 (2010)

Printed 16 July 2010

A (MN L TEX style file v2.2)

The kinematics of star-forming cores in Perseus ­ supporting online only material

Table 1. Dynamical properties of SCUBA clumps found with C L FI N D.

Sub-region NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC

a

Clump ID 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 1 2 3 4 5 6 7 8 9

b

Hatchell ID 42 43 44 41 45 46 48 50 47 51 52 49 ­ 56 54 55 62 60 65 ­ 63 ­ ­ 70 Bolo44 ­ 67 72 ­ ­ 74 ­ ­ ­ ­ ­ ­ ­ ­ 12 13 14 15 16 18 17 21 20

c

TNH3 (K) 13.5 16.3 16.5 15.0 16.4 14.3 15.0 14.8 14.4 12.3 16.4 12.4 12.0 23.0 15.0 11.7 15.0 11.7 12.5 12.0 13.3 12.0 12.0 15.5 13.6 12.0 15.0 10.6 12.0 12.0 10.8 12.0 12.0 12.0 12.0 11.3 12.0 12.0 12.0 12.9 14.2 16.0 11.7 13.0 11.1 12.9 10.0 10.9

d

vc (C18 O) (km s-1 ) 7.36 8.24 7.62 7.48 7.79 8.44 7.77 7.58 7.83 7.80 7.46 7.33 7.84 7.45 7.45 8.06 8.58 8.37 7.37 7.96 7.50 7.47 7.98 8.26 7.81 7.83 7.43 7.57 7.67 7.97 7.19 7.40 8.21 7.36 8.04 7.31 8.14 8.94 8.80 9.83 8.67 8.92 8.62 8.36 8.50 8.44

e

vC18 (km s

f O -1

)

NT g (km s-1 ) 0.81 0.64 0.50 0.77 0.59 0.52 0.43 0.88 0.70 0.79 0.77 0.25 0.40 0.53 0.43 0.34 0.52 0.45 0.81 0.75 0.40 0.63 0.58 0.56 0.72 0.40 0.40 0.39 0.57 0.82 0.30 0.17 0.51 0.18 0.49 0.15 0.45 0.33 0.35 0.64 0.35 0.33 0.42 0.31 0.29 0.35

Mvir h (M ) 11.3 11.9 12.3 13.7 22.9 8.3 5.8 11.2 12.8 17.3 9.8 2.2 11.3 4.9 3.7 6.8 10.1 4.3 3.1

1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333

1.91 1.53 1.19 1.81 1.40 1.23 1.01 2.08 1.65 1.86 1.82 0.60 0.95 1.26 1.03 0.82 1.24 1.07 1.92 1.78 0.95 1.49 1.37 1.32 1.71 0.96 0.94 0.92 1.36 1.94 0.71 0.43 1.20 0.44 1.16 0.38 1.07 0.78 0.83 1.52 0.83 0.79 1.01 0.74 0.68 0.83

11.3 6.1 4.7 1.9

3.6

IC348 IC348 IC348 IC348 IC348 IC348 IC348 IC348 IC348

4.3 3.6 9.3 4.9 2.8 2.1 5.5 1.3 3.5

c 2010 RAS


2

E. I. Curtis and J. S. Richer

Table 1 ­ continued Dynamical properties of SCUBA clumps found with C L FI N D. Sub-region IC348 IC348 IC348 IC348 IC348 IC348 IC348 IC348 IC348 IC348 IC348 IC348 IC348 IC348 L1448 L1448 L1448 L1448 L1448 L1448 L1448 L1448 L1448 L1448 L1448 L1448 L1448 L1448 L1448 L1448 L1455 L1455 L1455 L1455 L1455 L1455 L1455
a b a

Clump ID 10 11 12 13 14 15 16 17 18 19 20 21 22 23 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 1 2 3 4 5 6 7

b

Hatchell ID

c

TNH3 (K) 10.8 10.0 12.6 12.0 13.5 11.7 10.8 12.0 15.0 11.0 10.6 12.0 12.0 26.0 12.6 14.1 12.1 11.2 9.1 12.0 12.0 10.0 12.0 12.0 12.0 12.0 12.0 12.0 12.0 12.0 13.1 11.4 11.9 10.5 11.1 12.0 10.4

d

vc (C18 O) (km s-1 ) 9.49 8.83 8.73 8.63 8.53 8.76 9.17 9.12 8.65 8.07 8.79 9.05 9.01 8.27 4.47 5.16 4.07 4.07 4.35 4.73 4.11 3.87 3.89 3.53 4.24 4.39 4.93 4.21 4.74 4.83 5.19 5.16 5.86 6.13 4.57

e

vC18 (km s

f O -1

)

NT g (km s-1 ) 0.61 0.28 0.24 0.27 0.35 0.25 0.42 0.31 0.35 0.28 0.29 0.29 0.18 0.21 0.67 0.42 0.30 0.33 0.24 0.83 0.54 0.30 0.43 0.60 0.45 0.31 0.12 0.54 0.68 0.62 0.19 0.69 0.14 0.11 0.13

Mvir h (M ) 13.1 1.6 3.1 2.4 3.8 0.7 2.3

19 24 26 ­ 23 ­ 25 ­ Bolo101 ­ Bolo111 ­ ­ ­ 28 29 30 31 32 ­ ­ ­ ­ ­ ­ ­ ­ ­ ­ ­ 35 36 37 40 39 ­ ­

1.45 0.66 0.59 0.66 0.84 0.60 1.00 0.75 0.84 0.68 0.69 0.70 0.45 0.54 1.59 1.01 0.71 0.80 0.57 1.97 1.28 0.71 1.01 1.41 1.07 0.75 0.30 1.29 1.62 1.48 0.47 1.62 0.36 0.29 0.33

17.5 8.6 4.4 3.4 3.1

10.4 6.8 4.3 3.9 3.4

Name of sub-region map. Clump number from Curtis & Richer (2010). c H07 identifier. d Rosolowsky et al. (2008) NH kinetic temperature where they exist or 10.0, 15.0 and 12.0 K for starless clumps, protostars and clumps with no H07 3 identification where not respectively. e, f Measured C18 O J = 3 2 line centre velocity, v and FWHM, v c C18 O from a Gaussian fit to the line profile at the clump peak. These columns are left blank if there is no good fit or the line is too weak (< 3rms ). g Non-thermal contribution to the linewidth estimated using the temperatures of column (d). h Virial masses calculated using the temperatures of column (d). The virial masses have only been computed for clumps with a H07 association.

c 2010 RAS, MNRAS 000, 000­000


The kinematics of star-forming cores in the Perseus molecular cloud ­ supplement
Table 2. Dynamical properties of SCUBA clumps found with G AU S S C L U M P S. Sub-region NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC NGC
a

3

Clump ID 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 40 41 42 43 44 44 45 46 47 48 49 50 51 52 53 54 55 56 57 58 59 60 61 62

b

Hatchell ID 41,42 43 ­ 45 46 48 50 47 52 41 ­ 53 44 56 59 51 60 ­ 44 ­ ­ 57 ­ ­ 65 52 43 60 63 ­ 44 ­ 70 Bolo44 ­ ­ ­ ­ ­ ­ ­ ­ ­ ­ ­ ­ ­ 67 ­ ­ ­ 72 ­ 54 ­ ­ ­ ­ ­ ­ ­ ­ ­

c

TNH3 (K) 15.0 16.3 16.5 16.4 14.3 15.0 14.8 14.4 11.3 15.0 12.4 10.0 16.5 23.0 15.5 12.3 11.7 12.6 16.5 12.0 12.0 11.8 16.4 12.0 12.5 16.4 16.3 11.7 13.3 12.0 16.5 12.0 15.5 13.6 12.0 12.0 12.0 13.5 12.0 12.0 12.0 12.0 12.0 10.8 11.3 12.0 12.0 12.0 13.8 12.0 12.0 13.4 10.8 12.0 12.0 12.0 12.0 12.0 12.0 12.0 12.0 14.5 12.0

d

vc (C18 O) (km s-1 ) 6.77 8.18 7.62 7.82 8.40 7.78 7.58 7.78 7.67 7.80 7.34 7.65 7.32 7.44 7.81 7.70 8.12 8.51 7.65 7.75 7.53 7.36 7.86 8.70 7.95 7.73 8.40 8.40 7.50 8.45 7.88 7.98 8.30 7.95 8.50 8.41 7.80 6.74 8.02 7.97 8.48 7.64 7.86 7.79 7.79 7.83 7.07 7.43 7.66 7.55 7.58 7.40 7.36 7.66 7.93 8.73 8.67 8.12 8.17 7.73 7.40

e

vC18 (km s

f O -1

)

NT g (km s-1 ) 0.44 0.64 0.50 0.57 0.54 0.44 0.86 0.73 0.73 0.41 0.24 0.45 0.67 0.52 0.46 0.62 0.31 0.57 0.47 0.36 0.72 0.30 0.72 0.34 0.22 0.80 0.53 0.45 0.37 0.48 0.34 0.44 0.59 0.47 0.44 0.40 0.43 0.39 0.59 0.44 0.48 0.54 0.69 0.40 0.40 0.47 0.52 0.37 0.58 0.52 0.36 0.58 0.18 0.66 0.40 0.35 0.53 0.50 0.28 0.44 0.18

Mvir h (M ) 11.9 5.8 8.7 4.0 3.7 17.8 8.9 16.3 9.4 3.0 9.5 6.5 3.9 9.9 3.2 6.4

1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333 1333

1.04 1.51 1.19 1.35 1.27 1.05 2.02 1.72 1.71 0.97 0.58 1.06 1.59 1.24 1.08 1.46 0.75 1.36 1.11 0.86 1.71 0.71 1.71 0.82 0.54 1.89 1.26 1.08 0.89 1.15 0.81 1.04 1.40 1.12 1.03 0.94 1.01 0.94 1.39 1.05 1.13 1.29 1.63 0.94 0.94 1.12 1.23 0.89 1.38 1.24 0.87 1.37 0.45 1.57 0.94 0.83 1.25 1.18 0.67 1.04 0.46

1.8

6.4 6.5 3.9 4.1 1.2 8.7 6.6 5.3

3.2

1.4 2.4

c 2010 RAS, MNRAS 000, 000­000


4

E. I. Curtis and J. S. Richer

Table 2 ­ continued Dynamical properties of SCUBA clumps found with G AU S S C L U M P S. Sub-region
a

Clump ID 63 64 65 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25

b

Hatchell ID 51 ­ ­ 12 13 14 15 16 21 17 12 20 19 24,27 18

c

TNH3 (K) 14.8 12.0 12.0 12.9 14.2 16.0 11.7 11.1 10.0 12.9 12.9 10.9 10.8 13.5 13.0 12.0 10.8 12.0 12.0 12.0 10.5 12.0 12.0 12.0 11.0 10.6 10.0 12.6 14.1 12.1 11.1 11.2 12.6 12.0 9.1 14.1 15.0 12.0 12.0 12.1 12.0 14.1 11.2 12.0 12.0 12.0 10.0 12.0 12.0 12.0 12.1 12.0

d

vc (C18 O) (km s-1 ) 8.06 7.88 7.73 8.93 8.80 9.83 8.67 8.91 8.63 8.46 8.69 8.50 9.39 8.81 8.61 8.92 9.17 8.78 8.63 8.70 9.12 8.67 9.01 8.55 8.07 8.79 8.43 4.47 5.16 4.07 4.27 4.22 4.34 4.60 4.35 4.54 4.57 4.71 3.92 4.30 4.77 4.67 3.96 4.04 3.92 4.26 4.61 4.31 5.62

e

vC18 (km s

f O -1

)

NT g (km s-1 ) 0.95 0.53 0.41 0.32 0.35 0.64 0.35 0.33 0.30 0.41 0.41 0.28 0.47 0.27 0.34 0.20 0.42 0.30 0.31 0.48 0.31 0.36 0.32 0.50 0.29 0.29 0.27 0.62 0.42 0.30 0.44 0.28 0.41 0.29 0.23 0.77 0.42 0.41 0.26 0.42 0.35 0.38 0.57 0.20 0.30 0.44 0.20 0.24 0.06

Mvir h (M ) 2.7

NGC 1333 NGC 1333 NGC 1333 IC348 IC348 IC348 IC348 IC348 IC348 IC348 IC348 IC348 IC348 IC348 IC348 IC348 IC348 IC348 IC348 IC348 IC348 IC348 IC348 IC348 IC348 IC348 IC348 L1448 L1448 L1448 L1448 L1448 L1448 L1448 L1448 L1448 L1448 L1448 L1448 L1448 L1448 L1448 L1448 L1448 L1448 L1448 L1448 L1448 L1448 L1448 L1448 L1448

2.24 1.26 0.98 0.77 0.84 1.51 0.83 0.78 0.72 0.97 0.97 0.66 1.11 0.65 0.80 0.48 0.99 0.73 0.74 1.13 0.74 0.86 0.77 1.19 0.70 0.69 0.65 1.46 1.01 0.71 1.05 0.67 0.97 0.69 0.55 1.81 1.01 0.97 0.63 0.99 0.84 0.91 1.34 0.50 0.71 1.04 0.48 0.59 0.20

1.7 1.4 4.3 3.0 3.7 2.5 5.0 5.2 6.3 6.2 4.4 1.3 4.1

25 ­ ­ ­ Bolo113 101 ­ ­ ­ Bolo 111 21 27,28 29 30 ­ 31 28 ­ 32 29 27 ­ ­ ­ ­ 29 Bolo11 ­ ­ ­ ­ ­ ­ ­ 30 ­

5.1 0.9

2.9 0.4 7.1 2.2 1.3 3.1 8.0 2.3 11.2

4.2 7.5

3.4

c 2010 RAS, MNRAS 000, 000­000


The kinematics of star-forming cores in the Perseus molecular cloud ­ supplement
Table 2 ­ continued Dynamical properties of SCUBA clumps found with G AU S S C L U M P S. Sub-region L1455 L1455 L1455 L1455 L1455 L1455 L1455 L1455
a b a

5

Clump ID 1 2 3 4 5 6 7 8

b

Hatchell ID 35 36 37 40 39 ­ ­ ­

c

TNH3 (K) 13.1 11.4 11.9 10.5 15.0 12.0 12.0 12.0

d

vc (C18 O) (km s-1 ) 4.73 4.85 5.14 4.99 5.86 5.23 5.50

e

vC18 (km s

f O -1

)

NT g (km s-1 ) 0.62 0.38 0.23 0.42 0.18 0.56 0.22

Mvir h (M ) 3.1 4.8 1.4 4.1 0.9

1.46 0.90 0.57 1.01 0.45 1.34 0.53

Name of sub-region map. Clump number from Curtis & Richer (2010). c H07 identifier. d Rosolowsky et al. (2008) NH kinetic temperature where they exist or 10.0, 15.0 and 12.0 K for starless clumps, protostars and clumps with no H07 3 identification where not respectively. e, f Measured C18 O J = 3 2 line centre velocity, v and FWHM, v c C18 O from a Gaussian fit to the line profile at the clump peak. These columns are left blank if there is no good fit or the line is too weak (< 3rms ). g Non-thermal contribution to the linewidth estimated using the temperatures of column (d). h Virial masses calculated using the temperatures of column (d). The virial masses have only been computed for clumps with a H07 association.

c 2010 RAS, MNRAS 000, 000­000


6

E. I. Curtis and J. S. Richer

Table 3. Rotational properties of SCUBA clumps located with C L FI N D. These properties have been found by non-linear least squares fitting of a linear velocity gradient to the first moment of the C18 O J = 3 2 data. Only significant detections are shown with G /G 3. Sub-region NGC1333 NGC1333 NGC1333 NGC1333 NGC1333 NGC1333 NGC1333 NGC1333 NGC1333 NGC1333 NGC1333 NGC1333 NGC1333 NGC1333 NGC1333 NGC1333 IC348 IC348 IC348 IC348 IC348 IC348 IC348 L1448 L1448 L1448 L1448
a b c e f g h i a

Clump ID 2 3 5 6 8 9 10 11 13 16 17 18 25 26 27 29 1 2 3 4 7 10 21 1 2 4 7

b

Hatchell class I 0 I 0 I 0 S 0 S 0 0 S S I 0 0 0 I 0 S S 0 0 0

c

Number d of points 1117 2106 2229 978 330 872 936 408 685 711 662 1448 393 826 424 432 1271 777 643 1100 1071 731 499 1977 430 628 300

G ± G e (km s-1 pc-1 ) 3.16 ± 0.76 4.85 ± 0.35 1.54 ± 0.41 4.66 ± 0.84 10.63 ± 2.67 4.83 ± 0.74 8.98 ± 1.03 10.98 ± 2.15 4.13 ± 0.92 7.03 ± 1.02 7.00 ± 1.19 3.85 ± 0.39 3.77 ± 1.25 4.03 ± 0.85 4.66 ± 1.52 6.88 ± 1.90 6.43 3.78 4.43 3.17 4.13 8.06 5.29 ± ± ± ± ± ± ± 0 1 1 1 0 1 1 .73 .09 .26 .02 .44 .36 .30

G f (deg E of N) 155.44 26.88 21.10 125.79 -58.59 14.15 151.70 -20.48 -55.95 118.96 30.51 154.58 78.20 27.09 -21.04 78.74 -51.26 50.34 -77.63 4.14 -3.38 117.35 105.19 138.91 77.99 153.74 167.14

G /G 4 14 4 6 4 7 9 5 4 7 6 10 3 5 3 4 9 3 4 3 9 6 4 14 4 3 9

g



rot

h

ji (km s-1 pc) 1.05E-03 3.51E-03 1.63E-03 1.44E-03 9.83E-04 1.30E-03 2.90E-03 1.20E-03 1.08E-03 2.27E-03 1.52E-03 3.19E-03 4.63E-04 1.76E-03 1.03E-03 1.30E-03 2.32E-03 7.81E-04 7.95E-04 1.30E-03 1.94E-03 3.15E-03 9.83E-04 3.82E-03 2.35E-03 1.30E-03 5.21E-03

6.98E-04 5.39E-03 8.91E-04 3.35E-03 4.67E-03 2.91E-03 1.10E-02 5.90E-03 3.37E-03 1.22E-02 8.72E-03 9.50E-03 2.57E-03 8.02E-03 7.82E-03 1.36E-02 6.28E-03 1.49E-03 3.37E-03 3.33E-03 7.18E-03 4.50E-02 9.53E-03 3.61E-03 3.21E-03 1.97E-03 6.75E-02

5.67 ± 0.40 4.29 ± 1.12 3.45 ± 1.00 12.96 ± 1.38

Name of sub-region map. Clump identification from Curtis & Richer (2010). H07 clump class, S=starless, 0=Class 0 protostar and I=Class I protostar. d Number of points fitted in the map. Fitted velocity gradient and its error. Angle of the fitted velocity gradient, east of north. Level of significance of the fit, G /G . Ratio of the kinetic to gravitational energy. Specific angular momentum.

c 2010 RAS, MNRAS 000, 000­000


The kinematics of star-forming cores in the Perseus molecular cloud ­ supplement

7

Table 4. Rotational properties of SCUBA clumps located with G AU S S C L U M P S. These properties have been found by non-linear least squares fitting of a linear velocity gradient to the first moment of the C18 O J = 3 2 data. Only significant detections are shown with G /G 3. Sub-region NGC1333 NGC1333 NGC1333 NGC1333 NGC1333 NGC1333 NGC1333 NGC1333 NGC1333 NGC1333 NGC1333 NGC1333 NGC1333 NGC1333 NGC1333 NGC1333 NGC1333 NGC1333 NGC1333 NGC1333 NGC1333 NGC1333 NGC1333 NGC1333 IC348 IC348 IC348 IC348 IC348 IC348 IC348 IC348 IC348 IC348 L1448
a b c e f g h i a

Clump ID 1 4 7 8 9 12 15 16 17 18 20 21 26 33 34 35 39 41 44 47 50 58 63 64 4 5 6 7 10 14 17 18 22 23 18

b

Hatchell class 0 I I 0 0 S S S 0 0

c

Number d of points 800 922 1222 812 1374 531 840 624 918 800 661 251 959 627 485 466 356 775 1764 523 417 365 810 578 796 1259 586 1574 406 642 290 2158 909 908 405

G ± G e (km s-1 pc-1 ) 5.33 ± 1.33 4.93 ± 1.16 6.73 ± 0.84 4.25 ± 1.11 5.37 ± 0.65 4.97 ± 1.55 4.34 ± 0.90 8.12 ± 1.57 7.20 ± 0.88 5.23 ± 1.07 5.54 ± 1.42 16.04 ± 3.37 5.20 ± 1.20 12.12 ± 1.37 4.56 ± 1.37 7.73 ± 1.98 9.74 ± 2.94 4.38 ± 1.12 2.92 ± 0.43 13.80 ± 1.95 10.04 ± 2.53 9.17 ± 2.33 13.48 ± 1.01 7.53 ± 1.81 5.13 ± 1.17 2.54 ± 0.76 6.92 ± 1.57 5.47 ± 0.58 8.71 ± 2.37 3.40 ± 1.01 11.15 ± 2.83 3.62 ± 0.44 5.64 ± 1.08 3.81 ± 0.92 7.65 ± 0.85

G f (deg E of N) 135.67 -79.61 -77.95 26.44 -38.35 8.40 39.59 141.93 122.17 50.14 159.48 146.79 109.16 92.43 64.58 136.31 -24.36 175.36 -62.52 6.28 154.89 177.47 128.99 179.78 52.74 65.17 45.19 13.85 128.89 -32.47 -58.28 107.63 -47.00 149.83 163.01

G /G 4 4 8 4 8 3 5 5 8 5 4 5 4 9 3 4 3 4 7 7 4 4 13 4 4 3 4 9 4 3 4 8 5 4 9

g



rot

h

ji (km s-1 pc) 7.86E-04 7.41E-04 1.56E-03 5.54E-04 1.63E-03 4.46E-04 9.02E-04 9.34E-04 1.76E-03 9.99E-04 6.95E-04 3.71E-04 2.52E-03 1.79E-03 4.44E-04 6.99E-04 6.77E-04 9.51E-04 1.85E-03 1.40E-03 8.27E-04 6.70E-04 4.47E-03 1.05E-03 7.84E-04 6.87E-04 7.64E-04 2.09E-03 7.41E-04 5.21E-04 3.05E-04 2.54E-03 1.44E-03 9.72E-04 2.26E-03

0 S

I

6.90E-04 1.22E-03 4.27E-03 1.07E-03 3.70E-03 1.72E-03 2.91E-03 6.43E-03 8.90E-03 4.27E-03 3.46E-03 6.87E-03 2.10E-02 3.50E-02 3.15E-03 9.22E-03 1.31E-02 5.70E-03 5.07E-03 3.14E-02 1.68E-02 1.64E-02 1.48E-01 1.79E-02 3.55E-03 1.31E-03 6.09E-03 8.69E-03 1.20E-02 3.54E-03 6.48E-03 1.04E-02 1.55E-02 6.25E-03 2.54E-02

0 S S S S S S

Name of sub-region map. Clump identification from Curtis & Richer (2010). H07 clump class, S=starless, 0=Class 0 protostar and I=Class I protostar. d Number of points fitted in the map. Fitted velocity gradient and its error. Angle of the fitted velocity gradient, east of north. Level of significance of the fit, G /G . Ratio of the kinetic to gravitational energy. Specific angular momentum.

c 2010 RAS, MNRAS 000, 000­000


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E. I. Curtis and J. S. Richer
17:00

30

15:00

30

Declination 31:14:00 30

Declination

Declination

31:16:00

30

15:00

06

04

02 3:29:00 Right ascension

58

28:56

13:00

18:30

19:00

30

30

31:20:00

30

21:00

30

3:29:00

58

56

54 52 Right ascension

28:50

48

46

06

04

02

3:29:00

58

56

54

28:52

Right ascension

NGC 1333 2
30

NGC 1333 3
20
20 30

NGC 1333 5

31:19:00

10

31:16:00

Declination

Declination

Declination

50

30

40

30

18:00

20

15:10

19

18

17

16

15

14 13 Right ascension

12

11

3:29:10

09

3:29:10

09

08

07 Right ascension

06

05

21:00 04

10

20

30

40

50

31:22:00

10

02

3:29:00

58 Right ascension

56

28:54

NGC 1333 6
16:00

NGC 1333 8
20
30

NGC 1333 9

10

31:15:00

30

Declination

Declination

Declination

50

31:15:00

40

30

14:30

14:10

15

14

13

12

11 3:29:10 09 Right ascension

08

07

06

05

06.0

05.0

3:29:04.0 03.0 Right ascension

02.0

01.0

11:50 22

12:00

20

10

20

30

40

50

31:13:00

10

20

21

3:29:20

19

18 17 Right ascension

16

15

14

13

NGC 1333 10
18:00

NGC 1333 11
21:00

NGC 1333 13
30

30

40

20

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31:20:00

10

Declination

31:17:00

40

19:00

30

20

10

16:30

30

17:00

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46

44

42 3:28:40 Right ascension

38

36

11

3:29:10

09

08 07 Right ascension

06

05

04

44

42

3:28:40 38 Right ascension

36

34

32

18:00

10

20

30

40

Declination 50 31:19:00

Declination

31:18:00

Declination

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30

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20

06.0

05.0 3:29:04.0 Right ascension

03.0

02.0

NGC 1333 16 Figure 1. SCUBA 850 µm clumps scale denotes the C18 O J = 3 2 flux density are overlaid (black) at a white line positioned to show the

NGC 1333 17

NGC 1333 18

NGC 1333 25

identified with C L FI N D containing significant velocity gradients, G /G 3 in NGC 1333, IC348 and L1448. The colourline centre velocity, linearly scaled from the clump minimum (blue/black) to maximum (red/white). Contours of 850 µ m 100, 200, 400, 800, 1600 and 3200 mJy beam-1 . A white/black circle marks the position of the clump peak emission with direction of the fitted velocity gradient.

c 2010 RAS, MNRAS 000, 000­000


The kinematics of star-forming cores in the Perseus molecular cloud ­ supplement
16:00 10 25:00
30

9

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50

Declination

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40

Declination

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49

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45 44 Right ascension

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40

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14:00

32:00:00

30

30

01:00

24

23

22

21 3:29:20 Right ascension

19

18

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58

56

54 Right ascension

52

43:50

48

NGC 1333 26
40

NGC 1333 27
10

IC348 1

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32:02:00

30

Declination

Declination

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32:03:00

Declination

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30

50

20

00:50

01:00

40

02:30

02

01

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59

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57 Right ascension

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43:52

49

48

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42

41

02:30

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10

30

32:04:00

20

30

54

53

52

51 3:43:50 49 Right ascension

48

47

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45

IC348 2
30
30

IC348 3
50 01:00

IC348 4

32:05:00

31:59:00

Declination

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Declination

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04:00

58:00

03:30

02

3:44:00

58

56 Right ascension

54

52

43:50

42

41

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39

38 37 Right ascension

36

35

34

33

31:59:20 19

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17 3:44:16 Right ascension

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14

IC348 7
30 47:00
30

IC348 10
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IC348 21

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44:30

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42

40

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34 36 Right ascension

32

3:25:30

28

26

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38

36 Right ascension

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32

30

43:30

44:00

30

Declination 30:45:00

Declination

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Declination

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31

3:25:30

29 28 27 Right ascension

26

25

24

L1448 1
47:00

L1448 2

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Declination

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30 20

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30

18

16

14 Right ascension

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3:25:10

08

L1448 7 c 2010 RAS, MNRAS 000, 000­000 Figure 1 ­ continued


10

E. I. Curtis and J. S. Richer
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30

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3:29:10

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08

Right ascension

07 06 Right ascension

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NGC 1333 1
10

NGC 1333 4
16:00

NGC 1333 7
30 40 20:30 08 40 50 Declination 31:21:00 10 20

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Declination

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58

28:57

08

06

04 Right ascension

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28:58

07

06

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02

NGC 1333 8
30
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NGC 1333 9

NGC 1333 12

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Declination

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Declination

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Declination

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40

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17 15 3:29:16 Right ascension

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07

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50

30

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09

08 07 Right ascension

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NGC 1333 15
15:00

NGC 1333 16
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NGC 1333 17
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NGC 1333 18

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Declination 31:20:00 10

Declination

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09 08 Right ascension

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02.5 3:29:02.0 01.5 Right ascension

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02 3:29:00 Right ascension

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28:56

NGC 1333 20

NGC 1333 21

NGC 1333 26

Figure 2. SCUBA 850 µm clumps identified with G AU S S C L U M P S containing significant velocity gradients, G /G 3 in NGC1333, IC348 and L1448. The colour-scale denotes the C18 O J = 3 2 line centre velocity, linearly scaled from the clump minimum (blue/black) to maximum (red/white). Contours of 850 µ m flux density are overlaid (black) at 100, 200, 400, 800, 1600 and 3200 mJy beam-1 . A white/black circle marks the position of the clump peak emission with a white line positioned to show the direction of the fitted velocity gradient.

c 2010 RAS, MNRAS 000, 000­000


The kinematics of star-forming cores in the Perseus molecular cloud ­ supplement
21:00

11

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Declination 40 50 31:19:00

Declination 40 50

Declination

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40

10

19

18

17

16

3:29:15 Right ascension

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13

12

11

07.0

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3:29:05.0 04.0 Right ascension

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14 3:29:13 Right ascension

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11

NGC 1333 33
40

NGC 1333 34
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NGC 1333 35
20 30

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31:20:00

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40

30

Declination 10 20

Declination

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59.5

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57.5 3:28:57.0 56.5 Right ascension

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55.0

42

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39 38 Right ascension

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52

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48 46 Right ascension

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42

18:00 07.0

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Declination 40 50

Declination

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06.0

3:29:05.0 04.0 Right ascension

03.0

NGC 1333 39
10

NGC 1333 41
50

NGC 1333 44
10 19:40 50 31:20:00 10 Declination 20 30 40 50
Declination

NGC 1333 47

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40

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50

Declination

Declination 30 40

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30

19:20

13:00

07.0

06.0

3:29:05.0 04.0 Right ascension

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19.0

18.0

3:29:17.0 16.0 Right ascension

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14.0

15:10

20

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10

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21:00 14

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14

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11

3:29:10

09

08

07

06

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13

Right ascension

12 11 Right ascension

3:29:10

09

NGC 1333 50
04:00

NGC 1333 58

NGC 1333 63
30

NGC 1333 64

50

40

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30

Declination

32:02:00

Declination

Declination

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32:03:00

02:50

55

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53

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51 3:43:50 Right ascension

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48

47

01:00

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40

50

32:03:00

10

20

06

05

04

03

02 01 3:44:00 Right ascension

59

58

43:57

03

02

01

3:44:00 Right ascension

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58

43:57

IC348 4
05:00

IC348 5
20

IC348 6
32:01:00 20 Declination 30 40 50 01.0 10

Declination

Declination

32:04:00

30

58:10

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20

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30

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02

3:44:00

58 Right ascension

56

54

43:52

39.0

38.0

3:44:37.0 36.0 Right ascension

35.0

3:44:00.0 59.0 43:58.0 Right ascension

IC348 7 c 2010 RAS, MNRAS 000, 000­000

IC348 10 Figure 2 ­ continued

IC348 17


12

E. I. Curtis and J. S. Richer
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Declination

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Declination

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Declination

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10

28

26

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3:44:20 Right ascension

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09

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07

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3:44:05 04 Right ascension

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01

57:20 19

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40

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16