UBC 664

Click to load Aladin Lite
0.47 UTI
0.29
CN
0.41
Cdens
0.75
CC3
0.44
Clit
1.0
Cdup
Radius (P>50% members) 3.8 [arcmin]
  • CN 0.29 Poorly populated
  • Cdens 0.41 Loose
  • CC3 0.75 High quality
  • Clit 0.44 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
UBC 664 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is poorly studied in the literature.
Relatively close Moderate extinction Near-solar metallicity Very young

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

Cavallo et al. (2024)
Gold sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 226.11 -60.853 0.295 -4.39 -3.364 -38.261
Almeida et al. 2025 226.115 -60.874 – – – –
Hunt & Reffert 2024 226.116 -60.85 0.297 -4.44 -3.338 -74.823
Cavallo et al. 2024 226.104 -60.867 0.298 – – –
Hunt & Reffert 2023 226.116 -60.85 0.297 -4.44 -3.338 -74.823
Dias et al. 2021 226.115 -60.874 0.288 -4.349 -3.358 –
Cantat-Gaudin et al. 2020 226.132 -60.862 0.296 -4.362 -3.377 –
Castro-Ginard et al. 2020 226.125 -60.868 0.296 -4.353 -3.377 –

💡 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 3.27 2.02 – 11 – 430 – –
Hunt & Reffert 2024 – – – – – 563* – –
Cavallo et al. 2024 2.24 2.24 – 15 -0.330 – – –
Hunt & Reffert 2023 2.92 2.09 2.45 14 – – – –
Dias et al. 2021 3.27 2.02 – 11 0.356 – – –
Cantat-Gaudin et al. 2020 2.99 1.62 – 41 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

â„šī¸