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Table 1

Basic information of the SFR and YOCs investigated in this work.

Cluster RA Dec Age* Distance E(BV) 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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