OC 0521

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0.17 UTI
0.27
CN
0.18
Cdens
0.25
CC3
0.06
Clit
1.0
Cdup
Core radius and density 1.6 [pc], 0.9 [pc-2]
  • CN 0.27 Poorly populated
  • Cdens 0.18 Very loose
  • CC3 0.25 Low quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
OC 0521 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a moderate 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 age and metallicity parameters (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 P392, along with Gulliver_27.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.56 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.56 (50th percentile).

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 144.925 -54.043 0.354 -5.457 4.522 –
Hunt & Reffert 2024 144.965 -54.042 0.331 -5.429 4.502 –
Cavallo et al. 2024 144.748 -53.994 0.333 – – –
Hunt & Reffert 2023 144.965 -54.042 0.331 -5.429 4.502 –
Hao et al. 2022 144.956 -54.072 0.352 -5.539 4.563 –

💡 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– 2.68 2.74 1.97 33 0.374 306 – –
Hunt & Reffert 2024 2.68 2.69 1.97 33 – 306(1) – –
Cavallo et al. 2024 2.77 2.79 – 98 0.700 – – –
Hunt & Reffert 2023 2.68 2.69 1.97 33 – – – –
Hao et al. 2022 – 2.86 – 10 0.049 – – –

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

Visualization

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