OC 0339

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0.30 UTI
0.27
CN
0.37
Cdens
1.0
CC3
0.25
Clit
0.7
Cdup
Stellar density (N50/rad) 1.9 [N/pc2]
  • CN 0.27 Poorly populated
  • Cdens 0.37 Loose
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 0.7 Likely unique

Overview

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OC 0339 is a poorly populated, loose object of very high C3 quality. Its parallax locates it at a very close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Palma et al. (2025)
Part of multiple system G10, along with ASCC_19, ASCC_20, OCSN_61 and UBC_17a.

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 83.1 -0.477 2.753 1.586 -0.977 20.798
Hunt & Reffert 2024 83.119 -0.419 2.759 1.667 -1.028 29.1
Cavallo et al. 2024 83.271 -0.537 2.758 – – –
Hunt & Reffert 2023 83.119 -0.419 2.759 1.667 -1.028 29.1
Hao et al. 2022 83.047 -0.304 2.714 1.478 -0.863 –

💡 Note: The UCC values are estimated from its identified members.

Reference Year Dist [kpc] Av [mag] DAv [mag] Age [Myr] [Fe/H] [dex] Mass [Msun] Bfrac BSS
UCC 99999– 0.36 1.54 1.58 20 0.137 56 – –
Hunt & Reffert 2024 – – – – – 56(1) – –
Cavallo et al. 2024 0.37 1.37 – 20 0.000 – – –
Hunt & Reffert 2023 0.35 2.73 1.58 79 – – – –
Hao et al. 2022 – 1.54 – 6 0.274 – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 17 a 29.6 83.45 -1.71 2.76 1.61 -1.22 17.6 0.56
ASCC 19 3.7 82.05 -1.96 2.8 1.15 -1.22 19.28 0.96

💡 Note: The % column shows the percentage of members that OC 0339 shares with each listed object.

Visualization

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