OC 0453

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0.21 UTI
0.27
CN
0.29
Cdens
0.38
CC3
0.06
Clit
1.0
Cdup
Core radius and density 1.1 [pc], 1.5 [pc-2]
  • CN 0.27 Poorly populated
  • Cdens 0.29 Loose
  • CC3 0.38 Low quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
OC 0453 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a moderate distance, below 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 metallicity parameter (see Parameters). It is rarely studied in the literature.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Palma et al. (2025)
Classified as optical pair P33, along with HSC_2073.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.93 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.93 (50th percentile).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 125.067 -40.488 0.429 -4.046 4.011 –
Hunt & Reffert 2024 125.071 -40.48 0.431 -4.055 4.029 –
Cavallo et al. 2024 125.034 -40.477 0.429 – – –
Hunt & Reffert 2023 125.071 -40.48 0.431 -4.055 4.029 –
Hao et al. 2022 125.114 -40.501 0.443 -4.029 3.951 –

💡 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– 2.19 3.625 2.34 26 0.294 463 – –
Hunt & Reffert 2024 2.19 3.66 2.34 32 – 463(1) – –
Cavallo et al. 2024 2.68 3.59 – 19 0.540 – – –
Hunt & Reffert 2023 2.19 3.66 2.34 33 – – – –
Hao et al. 2022 – 1.47 – 6 0.049 – – –

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

Visualization

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