UBC 509

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0.04 UTI
0.27
CN
0.96
Cdens
0.75
CC3
0.3
Clit
0.07
Cdup
Stellar density (N50/rad) 4.8 [N/pc2]
  • CN 0.27 Poorly populated
  • Cdens 0.96 Very dense
  • CC3 0.75 High quality
  • Clit 0.3 Poorly studied
  • Cdup 0.07 Very likely duplicate

Overview

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UBC 509 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

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

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 99999– 164.118 -61.095 0.307 -6.574 2.411 –
Li et al. 2025 164.064 -61.089 0.287 -6.586 2.363 –
Almeida et al. 2025 164.051 -61.096 – – – –
Dias et al. 2021 164.051 -61.096 0.296 -6.568 2.358 –
Cantat-Gaudin et al. 2020 164.064 -61.089 0.287 -6.586 2.363 –
Castro-Ginard et al. 2020 164.048 -61.082 0.287 -6.571 2.373 –

💡 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– 3.24 0.85 – 193 0.258 372 – –
Li et al. 2025 3.14 0.79 – 78 0.263 – – –
Almeida et al. 2025 3.24 0.91 – 193 – 372 – –
Dias et al. 2021 3.24 0.91 – 193 0.253 – – –
Cantat-Gaudin et al. 2020 3.42 0.57 – 589 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
Collinder 236 92.6 164.12 -61.1 0.31 -6.56 2.43 2.41 0.76

💡 Note: The % column shows the percentage of members that UBC 509 shares with each listed object.

Visualization

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