UBC 1455

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0.39 UTI
0.34
CN
0.4
Cdens
0.62
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad) 2.0 [N/pc2]
  • CN 0.34 Poorly populated
  • Cdens 0.4 Loose
  • CC3 0.62 Intermediate quality
  • Clit 0.3 Poorly studied
  • Cdup 1.0 Unique

Overview

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UBC 1455 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, below 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.

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 99999– 131.112 -54.138 0.701 -3.501 6.602 28.661
Hu & Soubiran 2025 131.694 -54.638 – – – –
Hunt & Reffert 2024 131.002 -54.129 0.703 -3.535 6.636 28.596
Cavallo et al. 2024 131.694 -54.638 0.708 – – –
Hunt & Reffert 2023 131.002 -54.129 0.703 -3.535 6.636 28.596
Castro-Ginard et al. 2022 131.13 -54.13 0.7 -3.49 6.6 –

💡 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] Bfrac BSS
UCC 99999– 1.45 0.57 0.92 676 0.380 140 – –
Hu & Soubiran 2025 – – – – -0.120(5) – – –
Hunt & Reffert 2024 – – – – – 140(1) – –
Cavallo et al. 2024 1.68 0.57 – 676 0.880 – – –
Hunt & Reffert 2023 1.35 0.33 0.92 738 – – – –
Castro-Ginard et al. 2022 1.45 0.62 – 410 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 322 67.6 131.18 -54.16 0.72 -3.49 6.62 28.01 0.02

💡 Note: The % column shows the percentage of members that UBC 1455 shares with each listed object.

Visualization

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