UBC 91

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0.01 UTI
0.76
CN
1.0
Cdens
1.0
CC3
0.31
Clit
0.02
Cdup
Radius (P>50% members) 3.4 [arcmin]
  • CN 0.76 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.31 Poorly studied
  • Cdup 0.02 Very likely duplicate

Overview

â„šī¸
UBC 91 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age parameter (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 Moderate extinction Massive Near-solar metallicity Intermediate age

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

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 267.429 -28.759 0.44 -0.576 -1.147 -42.607
Li et al. 2025 267.433 -28.761 0.42 -0.587 -1.126 –
Almeida et al. 2025 267.454 -28.744 – – – –
Dias et al. 2021 267.454 -28.744 0.422 -0.585 -1.136 –
Cantat-Gaudin et al. 2020 267.433 -28.761 0.42 -0.587 -1.126 –
Castro-Ginard et al. 2020 267.422 -28.759 0.422 -0.587 -1.125 –

💡 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 1.65 1.37 – 650 0.025 – – –
Almeida et al. 2025 2.06 1.88 – 63 – 1036 – –
Dias et al. 2021 2.06 1.88 – 63 0.347 – – –
Cantat-Gaudin et al. 2020 2.20 1.28 – 229 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
Collinder 351 98.5 267.42 -28.75 0.45 -0.58 -1.14 -40.06 0.76

💡 Note: The % column shows the percentage of members that UBC 91 shares with each listed object.

Visualization

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