UPK 350

(OCSN 305)

Click to load Aladin Lite
0.68 UTI
0.62
CN
0.42
Cdens
1.0
CC3
0.69
Clit
1.0
Cdup
Radius (P>50% members) 46.7 [arcmin]
  • CN 0.62 Moderately populated
  • Cdens 0.42 Loose
  • CC3 1.0 Very high quality
  • Clit 0.69 Moderately studied
  • Cdup 1.0 Unique

Overview

UPK 350 is a moderately populated, loose object of very high C3 quality. Its parallax locates it at a very close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is moderately studied in the literature.
Very close Low extinction Near-solar metallicity Intermediate age

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

Hunt & Reffert (2024): Classified as a moving group.

Cavallo et al. (2024): Gold sample.

Data

Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 101.719 48.688 2.301 -4.882 -6.331 1.547
Almeida et al. 2025 101.742 48.684
Alfonso et al. 2024 101.635 48.954 2.27 -4.838 -6.322
Zhang et al. 2024 101.748 48.332
Cavallo et al. 2024 101.84 48.547 2.309
Hunt & Reffert 2023 101.747 48.332 2.318 -4.851 -6.343 2.09
Qin et al. 2023 101.64 48.59 2.29 -4.83 -6.33 1.57
He et al. 2022 101.617 48.828 2.309 -4.846 -6.318
Tarricq et al. 2022 101.646 48.722 2.308 -4.894 -6.307
Dias et al. 2021 101.742 48.684 2.23 -4.872 -6.375 5.613
Cantat-Gaudin et al. 2020 101.689 48.688 2.238 -4.845 -6.346
Sim et al. 2019 101.817 48.812 -4.88 -6.39

💡 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 0.45 0.43 516 80
Alfonso et al. 2024 0.46 0.19 53 -0.121
Zhang et al. 2024 -0.056*
Cavallo et al. 2024 0.47 0.51 72 0.000
Hunt & Reffert 2023 0.42 0.10 0.51 200
Qin et al. 2023 0.53 0.40 631
He et al. 2022 0.45 112
Tarricq et al. 2022 0.46 135
Dias et al. 2021 0.45 0.43 516 -0.121
Cantat-Gaudin et al. 2020 0.46 0.19 129
Sim et al. 2019 0.44 100

💡 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.

Visualization

Galactocentric position diagram

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