OC 0530

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0.18 UTI
0.27
CN
0.85
Cdens
0.75
CC3
0.06
Clit
0.44
Cdup
Core radius and density 0.8 [pc], 4.3 [pc-2]
  • CN 0.27 Poorly populated
  • Cdens 0.85 Dense
  • CC3 0.75 High quality
  • Clit 0.06 Rarely studied
  • Cdup 0.44 Possibly duplicate

Overview

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OC 0530 is a poorly populated, dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is rarely studied in the literature.

âš ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (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– 148.286 -57.399 0.342 -5.565 3.683 –
Hunt & Reffert 2024 148.28 -57.402 0.342 -5.543 3.661 –
Cavallo et al. 2024 148.274 -57.415 0.341 – – –
Hunt & Reffert 2023 148.28 -57.402 0.342 -5.543 3.661 –
Hao et al. 2022 148.243 -57.398 0.334 -5.546 3.703 –

💡 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– 2.69 1.88 0.66 30 0.158 425 – –
Hunt & Reffert 2024 2.69 1.88 0.66 30 – 425(1) – –
Cavallo et al. 2024 2.44 2.11 – 23 0.050 – – –
Hunt & Reffert 2023 2.69 1.88 0.66 30 – – – –
Hao et al. 2022 – 1.67 – 32 0.265 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 780 55.6 148.3 -57.41 0.35 -5.56 3.65 – 0.14

💡 Note: The % column shows the percentage of members that OC 0530 shares with each listed object.

Visualization

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