UBC 1366

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0.52 UTI
0.37
CN
0.98
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 4.9 [N/pc2]
  • CN 0.37 Poorly populated
  • Cdens 0.98 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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UBC 1366 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, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature.

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– 110.288 -12.61 0.36 -0.769 0.239 20.09
Hunt & Reffert 2024 110.312 -12.609 0.359 -0.77 0.249 44.908
Cavallo et al. 2024 110.285 -12.611 0.362 – – –
Hunt & Reffert 2023 110.312 -12.609 0.359 -0.77 0.249 44.908
Castro-Ginard et al. 2022 110.29 -12.62 0.36 -0.78 0.25 –

💡 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– 2.41 0.7 1.09 437 -0.140 204 – –
Hunt & Reffert 2024 – – – – – 204(1) – –
Cavallo et al. 2024 2.36 1.29 – 437 -0.140 – – –
Hunt & Reffert 2023 2.41 0.52 1.09 991 – – – –
Castro-Ginard et al. 2022 2.92 0.70 – 236 – – – –

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

Visualization

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