UBC 1351

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0.64 UTI
0.46
CN
1.0
Cdens
1.0
CC3
0.38
Clit
1.0
Cdup
Radius (P>50% members) 1.9 [arcmin]
  • CN 0.46 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.38 Poorly studied
  • Cdup 1.0 Unique

Overview

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UBC 1351 is a poorly 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, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.

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

Distant Low extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 107.733 -3.425 0.235 -0.336 0.022 63.802
Hu & Soubiran 2025 107.742 -3.415 – – – –
Zhang et al. 2024 107.726 -3.429 – – – –
Hunt & Reffert 2024 107.726 -3.429 0.226 -0.339 0.034 63.59
Cavallo et al. 2024 107.741 -3.415 0.228 – – –
Hunt & Reffert 2023 107.726 -3.429 0.226 -0.339 0.034 63.59
Castro-Ginard et al. 2022 107.76 -3.41 0.23 -0.31 0.03 –

💡 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
Hu & Soubiran 2025 – – – – -0.270* – – –
Zhang et al. 2024 – – – – -0.226* – – –
Hunt & Reffert 2024 – – – – – 397* – –
Cavallo et al. 2024 3.48 0.53 – 1122 0.130 – – –
Hunt & Reffert 2023 4.08 0.36 0.91 929 – – – –
Castro-Ginard et al. 2022 5.17 0.52 – 700 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 2965 65.2 107.73 -3.43 0.23 -0.35 0.06 63.8 0.11

💡 Note: The % column shows the percentage of members that UBC 1351 shares with each listed object.

Visualization

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