Table 4.
Characteristics of subregions.
| IRAS | CCD | CMD-1.88 kpc | CMD-6.1 kpc | Class I | Av | Mass limit | α slope | ||||
|---|---|---|---|---|---|---|---|---|---|---|---|
| Mem. | Class I | Mem. | Class I | Mem. | Class I | (mag) | Msun | ||||
| (%) | (%) | (%) | 1.88 kpc | 6.1kpc | |||||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) |
| 05184+3635 | 52 | 21 | 48 | 23 | 52 | 21 | 11 | 1.4 | 0.3–1.5 | 0.8–5 | 0.12 ± 0.04 |
| 05177+3636 | 79 | 28 | 65 | 34 | 79 | 28 | 22 | 1.34 | 0.2–2.2 | 0.7− > 7 | 0,2 ± 0.02 |
| 05168+3634 | 57 | 43 | 45 | 54 | 56 | 45 | 24 | 4.3 (4.5) | 0.5–2.5 | 0.9− > 7 | 0.21 ± 0.05 |
| 05162+3639 | 5 | − | 5 | − | 5 | − | 5 | 1.23 | − | − | − |
| 05156+3643 | 47 | 20 | 40 | 23 | 47 | 20 | 9 | 1.03 | 0.2–1.6 | 0.6–3 | 0.15 ± 0.04 |
Notes. (1) Name of subregions, (2) and (3) number of YSOs and the fraction of Class I objects (in percent) according to the color–color diagrams, (4)–(7) number of YSOs and the fraction of Class I objects (in percent) according to the color–magnitude diagrams in different distances, (8) number of Class I evolutionary stage objects, (9) interstellar extinction according to the COBE/DIRBE and IRAS/ISSA maps, (10)–(11) mass completeness limits of each subregion in two distances, (12) α slope of KLF of each subregion.
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