UBC 88

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0.01 UTI
0.76
CN
1.0
Cdens
0.75
CC3
0.4
Clit
0.02
Cdup
Stellar density (N50/rad) 14.3 [N/pc2]
  • CN 0.76 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.4 Poorly studied
  • Cdup 0.02 Very likely duplicate

Overview

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UBC 88 is a rich, very dense object of high C3 quality. Its parallax locates it at a close 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.

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.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 58.157 45.963 1.032 -1.438 -3.005 -10.819
Li et al. 2025 58.17 45.969 1.002 -1.421 -2.926 –
Alfonso et al. 2024 58.151 45.97 0.993 -1.415 -3.017 –
He et al. 2022 58.182 45.959 1.037 -1.452 -3.019 –
Cantat-Gaudin et al. 2020 58.17 45.969 1.002 -1.421 -2.926 –
Cantat-Gaudin & Anders 2020 58.17 45.969 1.002 -1.421 -2.926 –
Castro-Ginard et al. 2019 58.182 45.944 1.001 -1.359 -2.948 –

💡 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– 0.95 1.055 – 55 -0.030 – – –
Li et al. 2025 0.87 1.06 – 80 -0.040 – – –
Alfonso et al. 2024 0.95 1.05 – 63 -0.020 – – –
He et al. 2022 – 1.45 – 45 – – – –
Tarricq et al. 2022 0.93 – – 55 – – – –
Cantat-Gaudin et al. 2020 0.95 1.05 – 52 – – – –
Cantat-Gaudin & Anders 2020 0.97 – – – – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
UPK 322 100.0 58.16 45.96 1.03 -1.43 -3.02 -7.82 0.12
Teutsch 176 98.5 58.16 45.96 1.03 -1.44 -3.01 -10.82 0.62

💡 Note: The % column shows the percentage of members that UBC 88 shares with each listed object.

Visualization

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