UBC 633

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0.08 UTI
0.0
CN
0.18
Cdens
0.75
CC3
0.38
Clit
0.24
Cdup
Radius (P>50% members) 2.8 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.18 Very loose
  • CC3 0.75 High quality
  • Clit 0.38 Poorly studied
  • Cdup 0.24 Likely duplicate

Overview

â„šī¸
UBC 633 is a sparse, very loose object of high C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young 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 likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Very distant Moderate extinction Near-solar metallicity Very young

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 – 112.791 -15.432 0.176 -1.351 1.5 85.026
Li et al. 2025 112.824 -15.429 0.173 -1.343 1.477 –
Almeida et al. 2025 112.829 -15.434 – – – –
Celli et al. 2024 112.824 -15.429 – – – –
Dias et al. 2021 112.829 -15.434 0.178 -1.371 1.461 101.613
Cantat-Gaudin et al. 2020 112.824 -15.429 0.173 -1.343 1.477 –
Castro-Ginard et al. 2020 112.823 -15.442 0.173 -1.36 1.478 –

💡 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 5.79 1.60 – 534 0.241 – – –
Almeida et al. 2025 5.58 2.07 – 5 – 996 – –
Celli et al. 2024 – – – 14 – 228 – –
Dias et al. 2021 5.58 2.07 – 5 -0.100 – – –
Cantat-Gaudin et al. 2020 5.62 1.82 – 14 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
FSR 1234 76.0 112.79 -15.42 0.18 -1.32 1.54 85.03 0.51

💡 Note: The % column shows the percentage of members that UBC 633 shares with each listed object.

Visualization

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