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Table 1
Sample of resolved multiple protostellar systems (separation ≥7″).
System | Component | RA (J2000)a | Dec (J2000)a | Separationb (″) |
|
||||
L1448 C | N | 03:25:38.87 | +30:44:05.40 | ... |
... | S | 03:25:39.14 | +30:43:58.30 | 8.1 |
L1448 N | A | 03:25:36.53 | +30:45:21.35 | ... |
... | B | 03:25:36.34 | +30:45:14.94 | 7.3 |
... | C | 03:25:35.53 | +30:45:34.20 | 16.3 |
L1448 IRS2 | IRS2 | 03:25:22.40 | +30:45:12.00 | ... |
... | IRS2E | 03:25:25.66 | +30:44:56.70 | 46.9 |
NGC 1333 SVS13 | A | 03:29:03.75 | +31:16:03.76 | ... |
... | B | 03:29:03.07 | +31:15:52.02 | 14.9 |
... | C | 03:29:01.96 | +31:15:38.26 | 34.7 |
NGC 1333 IRAS 2 | A | 03:28:55.57 | +31:14:37.22 | ... |
... | B | 03:28:57.35 | +31:14:15.93 | 31.4 |
NGC 1333 IRAS 7 | Per18 | 03:29:11.26 | +31:18:31.08 | ... |
... | Per21 | 03:29:10.67 | +31:18:20.18 | 13.3 |
... | Per49 | 03:29:12.96 | +31:18:14.31 | 27.5 |
NGC 1333 IRAS 4 | B | 03:29:12.01 | +31:13:08.10 | ... |
... | B′ | 03:29:12.83 | +31:13:06.90 | 10.6 |
NGC 1333 IRAS 5 | Per52 | 03:28:39.72 | +31:17:31.89 | ... |
... | Per63 | 03:28:43.28 | +31:17:32.90 | 45.7 |
B1 Per6+Per10 | Per6 | 03:33:14.40 | +31:07:10.88 | ... |
... | Per10 | 03:33:16.45 | +31:06:52.49 | 31.9 |
IC 348 Per8+Per55 | Per8 | 03:44:43.94 | +32:01:36.09 | ... |
... | Per55 | 03:44:43.33 | +32:01:31.41 | 9.6 |
IC 348 MMS | Per11 | 03:43:57.06 | +32:03:04.60 | ... |
... | E | 03:43:57.73 | +32:03:10.10 | 10.2 |
IC 348 SMM2 | S | 03:43:51.08 | +32:03:08.32 | ... |
... | N | 03:43:51.00 | +32:03:23.76 | 16.1 |
B1-b | S | 03:33:21.30 | +31:07:27.40 | ... |
... | N | 03:33:21.20 | +31:07:44.20 | 17.4 |
... | W | 03:33:20.30 | +31:07:21.29 | 13.9 |
NGC 1333 Per58+Per65 | Per58 | 03:28:58.44 | +31:22:17.40 | ... |
... | Per65 | 03:28:56.31 | +31:22:27.80 | 28.9 |
IC 348 Per32+EDJ2009-366 | Per32 | 03:44:02.40 | +32:02:04.89 | ... |
... | EDJ2009-366 | 03:43:59.44 | +32:01:53.99 | 36.6 |
NGC 1333 PER37 | Per37 | 03:29:18.89 | +31:23:12.89 | ... |
... | EDJ2009-235 | 03:29:18.259 | +31:23:19.758 | 10.6 |
... | EDJ2009-233 | 03:29:17.675 | +31:22:44.922 | 33.7 |
Notes.
(a)
Coordinates from Tobin et al. (2016).
(b)
Separations are obtained from Tobin et al. (2016) and are listed relative to the first component tabulated. Typical uncertainties in position are <0.1″.
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