UBC 450

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0.46 UTI
0.58
CN
0.35
Cdens
0.75
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 6.8 [arcmin]
  • CN 0.58 Moderately populated
  • Cdens 0.35 Loose
  • CC3 0.75 High quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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UBC 450 is a moderately populated, loose 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 poorly studied in the literature.

Note: This object shares a small percentage of members with a later reported entry. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Young

Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 110.093 -19.374 0.323 -1.851 1.408 93.501
Almeida et al. 2025 110.118 -19.343 – – – –
Almeida et al. 2023 110.13 -19.343 – – – –
Dias et al. 2021 110.118 -19.343 0.312 -1.841 1.353 –
Cantat-Gaudin et al. 2020 110.103 -19.353 0.315 -1.844 1.367 –
Castro-Ginard et al. 2020 110.11 -19.33 0.312 -1.844 1.347 –

💡 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
Almeida et al. 2025 2.92 1.09 – 56 – 780 – –
Almeida et al. 2023 2.65 1.08 – 86 -0.130 632* 0.53 –
Dias et al. 2021 2.92 1.09 – 56 0.056 – – –
Cantat-Gaudin et al. 2020 3.03 0.72 – 69 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 268 12.1 109.97 -19.03 0.32 -1.69 1.48 49.45 0.09

💡 Note: The % column shows the percentage of members that UBC 450 shares with each listed object.

Visualization

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