OC 0467

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0.09 UTI
0.76
CN
1.0
Cdens
0.75
CC3
0.25
Clit
0.14
Cdup
Radius (P>50% members) 5.0 [arcmin]
  • CN 0.76 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 0.14 Likely duplicate

Overview

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OC 0467 is a rich, very dense object of high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is poorly studied in the literature.

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

Close Moderate extinction Near-solar metallicity Very young

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 – 129.403 -40.295 1.058 -5.668 3.694 19.988
Hunt & Reffert 2024 129.408 -40.292 1.054 -5.656 3.675 22.223
Cavallo et al. 2024 129.4 -40.289 1.058 – – –
Hunt & Reffert 2023 129.408 -40.292 1.054 -5.656 3.675 22.223
Hao et al. 2022 129.381 -40.288 1.083 -5.649 3.723 –

💡 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
Hunt & Reffert 2024 – – – – – 296* – –
Cavallo et al. 2024 0.96 1.20 – 2 -0.380 – – –
Hunt & Reffert 2023 0.88 1.07 2.11 4 – – – –
Hao et al. 2022 – 2.88 – 4 0.537 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 2221 85.6 129.43 -40.23 1.06 -5.62 3.77 21.57 0.41
CWNU 1239 3.0 129.85 -40.54 1.06 -5.38 3.47 -15.31 0.13

💡 Note: The % column shows the percentage of members that OC 0467 shares with each listed object.

Visualization

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