OC 0450

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0.50 UTI
0.25
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 7.0 [N/pc2]
  • CN 0.25 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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OC 0450 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a low-mass, near-solar metallicity, young cluster, but with a large variance across recent sources for the absorption and metallicity parameters (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.

Palma et al. (2025)
Classified as optical pair P609, along with CWNU_1083.

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 99999– 118.083 -42.462 3.021 -11.302 4.531 14.341
Hunt & Reffert 2024 118.138 -42.432 3.051 -11.398 4.659 10.139
Cavallo et al. 2024 119.172 -44.85 3.056 – – –
Hunt & Reffert 2023 118.138 -42.432 3.051 -11.398 4.659 10.139
Hao et al. 2022 118.027 -42.366 2.99 -11.037 4.606 15.607

💡 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– 0.325 0.47 0.47 22 0.271 40 – –
Hunt & Reffert 2024 – – – – – 40(1) – –
Cavallo et al. 2024 0.33 0.47 – 14 -0.070 – – –
Hunt & Reffert 2023 0.32 0.10 0.47 22 – – – –
Hao et al. 2022 – 2.93 – 32 0.611 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 14596 88.0 118.17 -42.47 3.03 -11.39 4.49 12.81 0.1

💡 Note: The % column shows the percentage of members that OC 0450 shares with each listed object.

Visualization

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