UBC 73

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0.01 UTI
0.74
CN
1.0
Cdens
0.75
CC3
0.31
Clit
0.01
Cdup
Radius (P>50% members) 5.1 [arcmin]
  • CN 0.74 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.31 Poorly studied
  • Cdup 0.01 Very likely duplicate

Overview

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UBC 73 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above 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.

Relatively close Low extinction Near-solar metallicity Intermediate age

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

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 95.384 26.925 0.441 0.421 -3.183 31.754
Li et al. 2025 95.381 26.913 0.448 0.455 -3.21 –
Almeida et al. 2025 95.377 26.921 – – – –
Dias et al. 2021 95.377 26.921 0.434 0.427 -3.206 –
Cantat-Gaudin et al. 2020 95.381 26.913 0.448 0.455 -3.21 –
Cantat-Gaudin & Anders 2020 95.381 26.913 0.448 0.455 -3.21 –

💡 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
Li et al. 2025 2.08 0.82 – 390 0.044 – – –
Almeida et al. 2025 2.03 1.13 – 218 – 602 – –
Dias et al. 2021 2.03 1.13 – 218 -0.185 – – –
Cantat-Gaudin et al. 2020 2.15 0.56 – 389 – – – –
Cantat-Gaudin & Anders 2020 2.10 – – – – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
Gulliver 56 99.0 95.38 26.92 0.44 0.44 -3.2 31.75 0.8
OC 0304 52.6 95.38 26.9 0.44 0.43 -3.18 27.53 0.0

💡 Note: The % column shows the percentage of members that UBC 73 shares with each listed object.

Visualization

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