Table 1
Observed sample.
| α2000 | δ2000 | Distance | |||||||
|---|---|---|---|---|---|---|---|---|---|
| IRAS source | (h m s) | (° ′ ′′) | Counterpart | Classif.(a) | Association(b) | HH in FOV | Location | (pc) | Ref. |
| I: Sources associated with jet emission | |||||||||
| 00087+5833 | 00 11 26.5 | + 58 49 50 | LkHα 198 | HAeBe | ⋯ | 161–164, 462 | L1265 | 344 ± 17 | 1 |
| 02236+7224 | 02 28 16.4 | + 72 37 36 | J02281661+7237328 | TT | RNO 7 (c) | 488 | L1340 | 861 ± 22 | 2 |
| 03220+3035 | 03 25 09.2 | + 30 46 21 | L1448-IRS1 | TT, b | RNO 13 (n) | 194–196 | L1448 | 240 ± 12 | 1 |
| 04073+3800 | 04 10 41.2 | + 38 07 54 | PP 13 | TT/FUO, b | PP 13 (n) | 463–465 | L1473 | 350 | 3 |
| 04239+2436 | 04 26 55.3 | + 24 43 34 | ⋯ | CI, b | ⋯ | 300 | Taurus | 129.0 ± 0.8 | 4 |
| 05380−0728 | 05 40 27.7 | − 07 27 28 | Re 50N | CI | ⋯ | 1121–1122 | L1641 | 460 | 5 |
| II: Sources with extended nebular emission | |||||||||
| 00044+6521 | 00 07 03.5 | + 65 38 41 | PP 1, McC H12 | HAeBe | ⋯ | ⋯ | Cepheus IV | 845 ± 110 | 6 |
| 05302−0537 | 05 32 41.7 | − 05 35 48 | J05324165−0535461 | CI, b | ⋯ | ⋯ | Orion A | 319 ± 12 | 2 |
| 05393+2235 | 05 42 21.3 | + 22 36 47 | J05422123+2236471 | FUO | RNO 54 (n) | ⋯ | ⋯ | 1540 ± 106 | 2 |
| 06249−1007 | 06 27 18.1 | − 10 09 41 | J06271812−1009387 | TT | HHL 43 (n) | ⋯ | ⋯ | 860 ± 70 | 7 |
| 06562−0337 | 06 58 44.4 | − 03 41 12 | J06584435−0341099 | HAeBe | Iron-clad Nebula | ⋯ | ⋯ | 5650 ± 430 | 7 |
| III: Point-like sources | |||||||||
| 00422+6131 | 00 45 09.9 | + 61 47 57 | J00450982+61147574 | TT | ⋯ | ⋯ | ⋯ |  |
2 |
| 02181+6817 | 02 22 22.6 | + 68 30 43 | CO Cas | HAeBe, v | ⋯ | ⋯ | ⋯ | 664 ± 25 | 2 |
| 05426+0903 | 05 45 22.4 | + 09 04 13 | FU Ori | FUO | ⋯ | ⋯ | ⋯ | 416 ± 9 | 2 |
| 06471−0329 | 06 49 40.4 | − 03 32 51 | J06494021−0332523 | CI | ⋯ | ⋯ | G216−2.5 | 2110 ± 21 | 1 |
Notes. (a) b: binary; CI: Class I; FUO: FU Ori; HAeBe: Herbig Ae/Be; TT: T Tauri; v: variable. (b) c: star cluster;n: extended nebular object.
References. (1) Zucker et al. (2020); (2) Gaia Collaboration (2018); (3) Cohen et al. (1983); (4) Galli et al. (2019); (5) Cohen (1990); (6) MacConnell (1968); (7) see text.
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