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Table 2

Derived physical parameters for the cores identified along filaments 8 and 10.

Filament No. RA Dec HL HS PA Rdec Mcore MBE Type
(J2000) (J2000) (″) (″) (°) (pc) (1021 cm−2) (M) (M)
29 04:21:14.5 +37:37:48 46.2 18.5 169.9 0.06 6.4(1) 0.9 1.1 R-PRE
30 04:21:14.6 +37:36:37 41.2 20 164.1 0.05 5(1.5) 0.9 1.1 R-PRE
F8 32 04:21:17.4 +37:35:38 37.8 20 116.5 0.05 4.3(1.7) 0.7 1 R-PRE
34 04:21:20.7 +37:34:51 39.1 20.5 165.8 0.05 2.4(1.2) 0.5 1 R-PRE
33 04:21:18.2 +37:33:44 37.6 19.8 4.8 0.05 11(1.4) 2.3 1 R-PRE

43 04:21:37.7 +37:35:21 32.5 18.2 157.4 0.04 5.6(2) 2.8 0.8 R-PRE
F10 44 04:21:38.5 +37:34:37 24.1 18.2 3 0.03 18.7(4.3) 3.8 0.5 PRO
46 04:21:41.1 +37:33:58 20.3 18.7 130.3 0.02 15.3(4.5) 1.9 0.3 PRO
49 04:21:45.5 +37:33:19 36.6 18.2 128.2 0.04 9(3.6) 2.9 0.9 R-PRE

Notes. This table shows the portion of Table A.1 corresponding to the cores along filaments 8 and 10. We note that No. is the core index number in Table A.1.; RA and Dec are the centroid equatorial coordinates of the cores. The cores are sorted from north to south along the crest of each filament. We note that HL and HS are the major and minor axes of the elliptical Gaussian source that was fit to each core in the Herschel high-resolution (18.2″) column density map; PA is the position angle of the major axis (measured east of north); Rdec is the deconvolved radius; is the peak column density; and Mcore is the mass estimated from an SED fitting. When a core is protostellar, Mcore is the protostellar envelope mass. Last, MBE is the critical Bonnor-Ebert (BE) mass, R-PRE stands for robust prestellar core, and PRO represents the protostellar core.

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