OC 0464

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0.45 UTI
0.26
CN
1.0
Cdens
0.38
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 1.7 [arcmin]
  • CN 0.26 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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OC 0464 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (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.

Relatively close Low extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 123.522 -43.099 0.571 -4.391 4.431 –
Hu & Soubiran 2025 123.532 -43.098 – – – –
Hunt & Reffert 2024 123.522 -43.096 0.562 -4.42 4.402 –
Cavallo et al. 2024 123.532 -43.098 0.563 – – –
Hunt & Reffert 2023 123.522 -43.096 0.562 -4.42 4.402 –
Hao et al. 2022 123.526 -43.082 0.566 -4.416 4.491 –

💡 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] Bfr BSS
Hu & Soubiran 2025 – – – – -0.260* – – –
Hunt & Reffert 2024 – – – – – 102* – –
Cavallo et al. 2024 1.72 0.73 – 537 0.370 – – –
Hunt & Reffert 2023 1.71 0.67 0.40 173 – – – –
Hao et al. 2022 – 1.94 – 63 0.611 – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 366 84.6 123.52 -43.1 0.57 -4.38 4.42 – 0.07

💡 Note: The % column shows the percentage of members that OC 0464 shares with each listed object.

Visualization

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