UBC 1322

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0.30 UTI
0.0
CN
0.13
Cdens
0.75
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 3.9 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.13 Very loose
  • CC3 0.75 High quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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UBC 1322 is a sparse, very loose object of high C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is poorly studied in the literature.
Very distant Low 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 – 101.525 12.009 0.189 0.004 -0.381 –
Zhang et al. 2024 101.544 12.053 – – – –
Hunt & Reffert 2024 101.544 12.053 0.188 0.011 -0.383 –
Cavallo et al. 2024 101.504 12.004 0.188 – – –
Hunt & Reffert 2023 101.544 12.053 0.188 0.011 -0.383 –
Castro-Ginard et al. 2022 101.52 11.97 0.19 -0.01 -0.38 –

💡 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
Zhang et al. 2024 – – – – -0.057* – – –
Hunt & Reffert 2024 – – – – – 222* – –
Cavallo et al. 2024 5.40 1.12 – 74 0.340 – – –
Hunt & Reffert 2023 4.58 0.51 1.64 316 – – – –
Castro-Ginard et al. 2022 5.34 0.71 – 39 – – – –

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

Visualization

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