UBC 1234

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0.36 UTI
0.38
CN
0.17
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 9.1 [arcmin]
  • CN 0.38 Poorly populated
  • Cdens 0.17 Very loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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UBC 1234 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.
Relatively close Moderate extinction Near-solar metallicity Young

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 – 30.863 58.828 0.4 -1.168 -0.851 -54.063
Hunt & Reffert 2024 30.801 58.89 0.401 -1.168 -0.849 -54.073
Cavallo et al. 2024 30.904 58.827 0.401 – – –
Hunt & Reffert 2023 30.801 58.89 0.401 -1.168 -0.849 -54.073
Castro-Ginard et al. 2022 30.85 58.84 0.4 -1.18 -0.85 –

💡 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
Hunt & Reffert 2024 – – – – – 282* – –
Cavallo et al. 2024 2.24 1.54 – 27 -0.260 – – –
Hunt & Reffert 2023 2.52 1.36 0.89 44 – – – –
Castro-Ginard et al. 2022 2.65 1.36 – 22 – – – –

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

Visualization

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