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Table A.1

Physical parameters of the cores identified with Herschel in the X-shaped nebula region.

No. RA Dec HL HS PA Rdec Mcore MBE Type
(J2000) (J2000) (″) (″) (°) (pc) (1021 cm−2) (M) (M)
1 04:19:20.6 +37:28:30 33.5 19.6 22.6 0.04 0.9 0.5 0.09 0.9 U-STA
2 04:19:26.7 +37:21:50 40.9 18.2 40.4 0.05 0.7 0.3 0.3 1 C-PRE
3 04:19:27.7 +37:28:05 62.9 42.1 140.2 0.12 0.7 0.4 0.2 2.3 U-STA
4 04:19:28.7 +37:20:34 51 34.8 86.1 0.09 1.2 0.7 0.5 1.8 U-STA
5 04:19:29.7 +37:22:50 52 23.5 17.6 0.07 1.1 0.5 0.5 1.4 C-PRE
6 04:19:36.4 +37:29:05 27.8 18.2 128.5 0.03 0.8 0.3 0.2 0.6 C-PRE
7 04:19:36.7 +37:28:46 26.3 18.2 133.8 0.03 0.7 0.3 0.1 0.6 U-STA
8 04:19:37.2 +37:26:48 52.3 36.3 102 0.1 2.2 0.8 1.4 1.9 R-PRE
9 04:19:39.8 +37:28:59 48.8 35.5 85.7 0.09 1.2 0.4 1.2 1.8 R-PRE
10 04:19:49.5 +37:24:01 34.5 24.3 151.2 0.05 0.8 0.5 0.2 1.1 U-STA
11 04:19:57.5 +37:31:06 43.4 23.4 95 0.06 1.1 0.3 0.3 1.3 C-PRE
12 04:20:03.7 +37:31:24 50.6 18.4 52.4 0.06 1.5 0.5 4.4 1.2 R-PRE
13 04:20:14.8 +37:31:53 49.2 32.1 84.9 0.09 2.9 1.1 1.1 1.7 R-PRE
14 04:20:26.4 +37:10:25 37.7 25.1 49.6 0.06 1.2 0.8 0.2 1.2 U-STA
15 04:20:30.6 +37:33:31 46.3 21.8 85.7 0.06 0.6 0.3 0.1 1.3 U-STA
16 04:20:33.3 +37:12:09 44.1 25.2 0.1 0.07 0.4 0.3 0.1 1.3 U-STA
17 04:20:34.9 +37:15:38 40.7 20.6 2.6 0.05 0.2 0.1 0.06 1.1 U-STA
18 04:20:42.1 +37:33:32 31.4 21.9 83.9 0.05 1.4 0.8 0.6 0.9 R-PRE
19 04:20:45.5 +37:29:49 38.1 25.6 57.9 0.06 1.1 0.6 0.3 1.2 U-STA
20 04:20:47.4 +37:30:38 44.5 35.9 38.5 0.09 1.5 0.8 2.2 1.7 R-PRE
21 04:20:47.8 +37:17:16 77.5 26.5 40.4 0.1 0.7 0.3 0.5 2 U-STA
22 04:20:53.9 +37:33:12 54.3 24.8 94.4 0.08 0.8 0.3 0.3 1.5 U-STA
23 04:21:00.6 +37:32:41 31.1 20.6 55.6 0.04 1.5 0.4 0.2 0.8 C-PRE
24 04:21:00.9 +37:31:19 28.6 20.6 97.6 0.04 0.5 0.2 0.04 0.8 U-STA
25 04:21:01.2 +37:20:50 53.6 31.9 4.8 0.09 4.8 1.6 5.8 1.8 R-PRE
26 04:21:02.8 +37:34:24 43.6 31.7 5.4 0.08 0.9 0.4 0.2 1.6 U-STA
27 04:21:05.8 +37:24:12 42.3 33.6 33.3 0.08 1.4 0.6 0.5 1.6 C-PRE
28 04:21:07.3 +37:25:20 52.3 30.5 37.1 0.09 2.2 0.8 1.3 1.7 R-PRE
29 04:21:14.5 +37:37:48 46.2 18.5 169.9 0.06 6.3 1.4 0.9 1.1 R-PRE
30 04:21:14.6 +37:36:37 41.2 20 164.1 0.05 5 0.9 0.9 1.1 R-PRE
31 04:21:15.5 +37:31:49 23.8 18.2 7.8 0.02 0.9 0.2 0.2 0.5 C-PRE
32 04:21:17.4 +37:35:38 37.8 20 116.5 0.05 4.3 0.5 0.7 1 R-PRE
33 04:21:18.2 +37:33:44 37.6 19.8 4.8 0.05 10.9 1.1 2.3 1 R-PRE
34 04:21:20.7 +37:34:51 39.1 20.5 165.8 0.05 2.4 0.3 0.5 1 R-PRE
35 04:21:23.3 +37:32:20 22.4 18.7 90.3 0.02 0.7 0.1 0.05 0.5 U-STA
36 04:21:24.4 +37:36:31 53 21.9 52.4 0.07 0.9 0.3 0.4 1.4 C-PRE
37 04:21:26.2 +37:36:38 22.5 18.2 41.9 0.02 0.5 0.2 0.07 0.4 U-STA
38 04:21:29.9 +37:33:24 51.8 42.8 87.7 0.11 2.4 0.5 0.8 2.1 C-PRE
39 04:21:32.7 +37:42:23 50.4 36.4 5.4 0.09 0.6 0.5 0.2 1.9 U-STA
40 04:21:33.7 +37:32:54 34.1 18.2 92.7 0.04 3.6 0.4 0.6 0.8 R-PRE
41 04:21:35.6 +37:36:22 26.6 18.2 138.4 0.03 0.8 0.1 0.4 0.6 R-PRE
42 04:21:37.4 +37:37:43 33.3 23 69.2 0.05 1.1 0.3 0.1 1 U-STA
43 04:21:37.7 +37:35:21 32.5 18.2 157.4 0.04 5.6 0.6 2.8 0.8 R-PRE
44 04:21:38.5 +37:34:37 24.1 18.2 3 0.03 18.7 1.9 3.8 0.5 PRO
45 04:21:39.2 +37:32:31 45.9 18.3 136.4 0.05 4.3 0.5 0.3 1.1 C-PRE
46 04:21:41.1 +37:33:58 20.3 18.7 130.3 0.02 15.3 1.2 1.9 0.3 PRO
47 04:21:41.3 +37:37:16 27.2 22.1 116.7 0.04 0.9 0.2 0.1 0.8 U-STA
48 04:21:45.2 +37:32:15 31 23.2 2.3 0.05 1.7 0.2 0.6 1 R-PRE
49 04:21:45.5 +37:33:19 36.6 18.2 128.2 0.04 9 0.9 2.9 0.9 R-PRE
50 04:21:50.6 +37:32:32 28.7 18.2 163.8 0.03 1.3 0.2 0.5 0.7 R-PRE
51 04:21:51.2 +37:32:03 22.6 18.2 164.9 0.02 1.4 0.3 0.3 0.4 R-PRE
52 04:21:55 +37:31:43 27.6 22.7 133.5 0.04 1 0.3 0.2 0.8 C-PRE
53 04:21:55.2 +37:38:04 43.8 18.2 22.6 0.05 0.5 0.3 0.1 1 U-STA
54 04:21:57.7 +37:20:10 59.7 29 14.4 0.09 0.5 0.3 0.2 1.8 U-STA
55 04:22:02.8 +37:34:17 34.2 18.2 111.3 0.04 0.7 0.5 0.2 0.8 U-STA
56 04:22:07.4 +37:16:49 53.6 32 166.5 0.09 0.9 0.5 0.3 1.8 U-STA
57 04:22:09.7 +37:14:39 45.8 35.7 90.2 0.09 1 0.5 0.3 1.7 U-STA

Notes. These cores were identified and classified using the standard HGBS procedure described by Könyves et al. (2015). We note that RA and Dec are the centroid equatorial coordinates of the cores, and the cores are sorted from west to east; 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 core radius; is the peak column density; is the ratio of the peak to background column density; and Mcore is the core mass estimated from SED fitting. When a core is protostellar, Mcore is the protostellar envelope mass. Last MBE is the critical Bonnor-Ebert (BE) mass and R-PRE, C-PRE, U-STA, and PRO stand for the robust prestellar core, the candidate prestellar core, the unbound starless core, and the protostellar core, respectively. There are 24 U-STA cores, 11 C-PRE cores, 20 R-PRE cores, and two PRO cores in total.

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