Table 1
Source list.
| Source | Other | RA, Dec (J2000)a | Energetic | Source | Dist. | Region | Ref. |
| names | [h:m:s, °:′:″] | statusb | notesc | [pc] | |||
|
|
|||||||
| CB 4-SMM | ... | 00:39:05.2, +52:51:47 | sub-critical | 1 | 350 ± 150 | Cas A, Gould’s Belt (GB) | 1, 2 |
| CB 17-SMMc | L 1389 | 04:04:37.1, +56:56:02 | ~stable | 2, 3 | 250 ± 50 | Perseus, GB | 2, 3, 1 |
| CB 26-SMM2d | L 1439 | 05:00:14.5, +52:05:59 | ~stable | 2, 4 | 140 ± 20 | Auriga | 2, 3, 4, 5 |
| CB 27-SMM | L 1512-S | 05:04:08.1, +32:43:30 | ~stable | 1 | 140 ± 20 | Taurus-Auriga | 2, 4, 5 |
| B 68-SMM | L 57, CB 82 | 17:22:38.3, −23:49:51 | ~stable | 1 | 135 ± 15 | Ophiuchus, Pipe nebula | 2, 6, 7, 8 |
| CB 244-SMM2e | L 1262 | 23:25:26.8, +74:18:22 | super-critical | 2, 5 | 200 ± 30 | Cepheus flare, GB | 2, 3, 4, 9 |
Notes.
Position of the column density peak of the starless core as derived in Launhardt et al. (2013).
Source notes: 1: single-core globule, 2: double-core globule, 3: CB 17 contains an additional low-luminosity Class I YSO (IRS) located 25″ from starless core (SMM), not embedded, but partially blending, 4: CB 26 contains an additional Class I YSO (SMM1) located 3.6′ south-west of the starless core (SMM2), 5: CB 244 contains an additional Class 0 source (SMM1) located ~90″ east of starless core (SMM2), partially blending.
Reference. (1) Perrot & Grenier (2003); (2) Launhardt et al. (2013); (3) Launhardt et al. (2010); (4) Loinard et al. (2011); (5) Stutz et al. (2009); (6) de Geus et al. (1989); (7) Lombardi et al. (2006); (8) Alves & Franco (2007); (9) Kun (1998).
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