OC 0606

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0.40 UTI
0.0
CN
1.0
Cdens
0.38
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad) 10.2 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.3 Poorly studied
  • Cdup 1.0 Unique

Overview

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OC 0606 is a sparse, very dense object of low C3 quality. Its parallax locates it at a relatively close distance, near 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 absorption and age parameters (see Parameters). It is poorly studied in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Liu et al. (2025)
Classified as primordial binary cluster 312 along with Theia_339.

Palma et al. (2025)
Classified as optical pair (not dynamically associated) P243, along with Theia_339.

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– 212.866 -63.149 0.519 -5.148 -2.882 –
Hunt & Reffert 2024 212.897 -63.141 0.508 -5.141 -2.888 –
Cavallo et al. 2024 212.906 -63.139 0.507 – – –
Hunt & Reffert 2023 212.897 -63.141 0.508 -5.141 -2.888 –
Hao et al. 2022 212.897 -63.146 0.535 -5.181 -2.83 –

💡 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– 2.08 1.06 0.64 98 -0.074 227 – –
Liu et al. 2025 3.08 0.47 – 76 – – – –
Hunt & Reffert 2024 – – – – – 227(1) – –
Cavallo et al. 2024 2.08 0.73 – 617 -0.200 – – –
Hunt & Reffert 2023 1.79 1.39 0.64 118 – – – –
Hao et al. 2022 – 1.94 – 79 0.051 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 247 100.0 212.92 -63.13 0.52 -5.14 -2.89 – 0.22

💡 Note: The % column shows the percentage of members that OC 0606 shares with each listed object.

Visualization

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