UBC 204

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0.00 UTI
0.55
CN
1.0
Cdens
1.0
CC3
0.25
Clit
0.0
Cdup
Radius (P>50% members) 1.3 [arcmin]
  • CN 0.55 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 0.0 Very likely duplicate

Overview

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UBC 204 is a moderately populated, very dense object of very 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, very 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.

Distant Low extinction Near-solar metallicity Very young

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 102.37 12.037 0.203 0.047 -0.399 37.257
Li et al. 2025 102.371 12.045 0.199 0.108 -0.392 –
Celli et al. 2024 102.367 12.046 – – – –
Cantat-Gaudin et al. 2020 102.371 12.045 0.199 0.108 -0.392 –
Castro-Ginard et al. 2020 102.379 12.058 0.205 0.091 -0.394 –

💡 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 4.36 0.93 – 22 -0.130 – – –
Celli et al. 2024 – – – 15 – 323 – –
Cantat-Gaudin et al. 2020 4.61 0.73 – 15 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
Juchert J0649.4+1202 100.0 102.37 12.04 0.21 0.04 -0.41 28.9 0.59

💡 Note: The % column shows the percentage of members that UBC 204 shares with each listed object.

Visualization

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