UBC 345

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0.50 UTI
0.42
CN
0.72
Cdens
0.75
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 5.5 [arcmin]
  • CN 0.42 Poorly populated
  • Cdens 0.72 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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UBC 345 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is poorly studied in the literature.

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

Relatively close High extinction Near-solar metallicity Very young

Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 276.031 -12.237 0.469 -0.426 -1.703 -63.452
Almeida et al. 2025 275.966 -12.238 – – – –
Celli et al. 2024 276.005 -12.256 – – – –
Dias et al. 2021 275.966 -12.238 0.464 -0.457 -1.715 –
Cantat-Gaudin et al. 2020 276.005 -12.256 0.472 -0.452 -1.706 –
Castro-Ginard et al. 2020 275.995 -12.268 0.472 -0.455 -1.713 –

💡 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 2.04 3.40 – 8 – 657 – –
Celli et al. 2024 – – – 14 – 477 – –
Dias et al. 2021 2.04 3.40 – 8 0.230 – – –
Cantat-Gaudin et al. 2020 2.00 3.38 – 14 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 2334 59.5 276.04 -12.24 0.45 -0.35 -1.7 -32.63 0.23

💡 Note: The % column shows the percentage of members that UBC 345 shares with each listed object.

Visualization

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