UPK 108

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0.15 UTI
0.39
CN
0.27
Cdens
0.75
CC3
0.44
Clit
0.33
Cdup
Radius (P>50% members) 21.7 [arcmin]
  • CN 0.39 Poorly populated
  • Cdens 0.27 Loose
  • CC3 0.75 High quality
  • Clit 0.44 Poorly studied
  • Cdup 0.33 Possibly duplicate

Overview

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UPK 108 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.

âš ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Close Low extinction Near-solar metallicity Young

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

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 315.461 29.744 1.178 1.032 -4.787 -11.955
Li et al. 2025 315.551 29.997 1.173 1.073 -4.748 –
Almeida et al. 2025 315.669 29.898 – – – –
Alfonso et al. 2024 315.278 29.598 1.145 0.954 -4.857 –
Dias et al. 2021 315.669 29.898 1.169 1.048 -4.74 –
Cantat-Gaudin et al. 2020 315.551 29.997 1.173 1.073 -4.748 –
Cantat-Gaudin & Anders 2020 315.551 29.997 1.167 1.027 -4.738 –
Sim et al. 2019 315.521 29.79 – 1.02 -4.72 –

💡 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 0.80 0.27 – 42 0.057 – – –
Almeida et al. 2025 0.82 0.44 – 120 – 66 – –
Alfonso et al. 2024 0.82 0.27 – 61 -0.008 – – –
Dias et al. 2021 0.82 0.44 – 120 -0.008 – – –
Cantat-Gaudin et al. 2020 0.82 0.27 – 41 – – – –
Cantat-Gaudin & Anders 2020 0.84 – – – – – – –
Sim et al. 2019 0.84 – – 45 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
Teutsch 312 66.7 315.44 29.67 1.17 1.01 -4.8 -10.24 0.42

💡 Note: The % column shows the percentage of members that UPK 108 shares with each listed object.

Visualization

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