UBC 1396

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0.51 UTI
0.32
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 10.3 [N/pc2]
  • CN 0.32 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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UBC 1396 is a poorly populated, very dense object of 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 (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– 118.5 -26.76 0.231 -2.463 3.233 –
Hunt & Reffert 2024 118.502 -26.76 0.233 -2.452 3.24 –
Cavallo et al. 2024 118.507 -26.765 0.233 – – –
Hunt & Reffert 2023 118.502 -26.76 0.233 -2.452 3.24 –
Castro-Ginard et al. 2022 118.48 -26.77 0.25 -2.47 3.24 –

💡 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– 3.99 0.81 0.67 110 -0.480 347 – –
Hunt & Reffert 2024 – – – – – 347(1) – –
Cavallo et al. 2024 3.10 0.90 – 110 -0.480 – – –
Hunt & Reffert 2023 3.99 0.71 0.67 156 – – – –
Castro-Ginard et al. 2022 5.38 0.81 – 94 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 8833 75.0 118.49 -26.76 0.24 -2.38 3.32 – 0.21

💡 Note: The % column shows the percentage of members that UBC 1396 shares with each listed object.

Visualization

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