Table 1
Basic information of the SFR and YOCs investigated in this work.
Cluster | RA | Dec | Age* | Distance | ![]() |
E(B−V) | Ref. | |||
---|---|---|---|---|---|---|---|---|---|---|
(J2000) | (J2000) | (Myr) | (pc) | (kpc) | (mag) | |||||
IC 2391 | 08 40 32.00 | −53 02 00.00 | 50 ± 30 | 151 ± 2 | 8.00 ± 0.01 | <0.05 | 1, 2 | |||
IC 2602 | 10 42 58.00 | −64 24 00.00 | 30 ± 20 | 152 ± 3 | 7.95 ± 0.01 | 0.02-0.04 | 3 | |||
IC 4665 | 17 46 18.00 | +05 43 00.00 | 40 ± 10 | 345 ± 12 | 7.72 ± 0.01 | 0.16-0.19 | 4 | |||
NGC 2264 | 06 40 58.00 | +09 53 42.00 | 3-5 ± 4** | 723 ± 57 | 8.66 ± 0.13 | 0.075 | 5, 6 | |||
NGC 2516 | 07 58 04.00 | −60 45 12.00 | 130 ± 60 | 409 ± 18 | 7.98 ± 0.01 | 0.11 | 7 | |||
NGC 2547 | 08 10 25.70 | −49 10 03.00 | 50 ± 20 | 387 ± 15 | 8.05 ± 0.01 | 0.12 | 8 |
Notes. The clusters are sorted by name. The distances (fifth column) are from Cantat-Gaudin et al. (2018). The asterisk indicates ages and Galactocentric distances (RGal) from Netopil et al. (2016). We adopted RGal,⊙ = 8.00 kpc. The double asterisk indicates the age value from Venuti et al. (2018).
References. (1) Barrado y Navascues et al. (1999); (2) Barrado y Navascués et al. (2004); (3) van Leeuwen (2009); (4) Cargile & James (2010); (5) Sung et al. (2004); (6) Turner (2012); (7) Bailey et al. (2018); (8) Naylor & Jeffries (2006).
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