UBC 33

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0.58 UTI
0.62
CN
0.9
Cdens
0.75
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 9.0 [arcmin]
  • CN 0.62 Moderately populated
  • Cdens 0.9 Very dense
  • CC3 0.75 High quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

UBC 33 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Data

Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 7.399 60.512 0.646 -0.946 -0.51 -31.802
Hunt & Reffert 2024 7.325 60.471 0.646 -0.937 -0.547 -36.855
Cavallo et al. 2024 7.436 60.508 0.647
Hunt & Reffert 2023 7.325 60.471 0.646 -0.937 -0.547 -36.855
Cantat-Gaudin et al. 2020 7.36 60.498 0.627 -0.928 -0.443
Castro-Ginard et al. 2019 7.394 60.491 0.626 -0.94 -0.456

💡 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
Hunt & Reffert 2024 403*
Cavallo et al. 2024 1.48 1.77 166 0.190
Hunt & Reffert 2023 1.46 1.65 1.33 74
Cantat-Gaudin et al. 2020 1.58 1.54 138

💡 Note: The parameters are sometimes transformed from their original values to match the format of the columns shown here, see FAQ. The columns DAv, Bfr, BSS correspond to differential extinction, binary fraction, and blue stragglers, respectively. BSS values can be listed as fractions or integers.
(*): indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 14133 78.4 7.38 60.51 0.65 -0.95 -0.53 -31.15 0.02

💡 Note: The % column shows the percentage of members that UBC 33 shares with each listed object.

Visualization

Galactocentric position diagram

💡 Note: How are the galactocentric plots generated? See FAQ.