OC 0026

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0.50 UTI
0.0
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 5.2 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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OC 0026 is a sparse, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is poorly studied in the literature.

Palma et al. (2025)
Classified as optical pair P135, along with HSC_176.

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– 274.947 -16.513 0.566 0.142 -1.729 19.141
Hunt & Reffert 2024 274.92 -16.541 0.553 0.166 -1.687 –
Cavallo et al. 2024 274.923 -16.53 0.554 – – –
Hunt & Reffert 2023 274.92 -16.541 0.553 0.166 -1.687 –
Hao et al. 2022 274.938 -16.536 0.568 0.103 -1.767 –

💡 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– 1.69 4.24 2.89 46 0.285 533 – –
Hunt & Reffert 2024 – – – – – 533(1) – –
Cavallo et al. 2024 1.66 4.17 – 100 0.520 – – –
Hunt & Reffert 2023 1.72 4.24 2.89 46 – – – –
Hao et al. 2022 – 4.78 – 3 0.051 – – –

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

Visualization

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