UBC 1072

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0.64 UTI
0.69
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.0 [arcmin]
  • CN 0.69 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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UBC 1072 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.
Distant Moderate extinction Massive 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 – 297.875 29.842 0.216 -3.422 -6.351 –
Hunt & Reffert 2024 297.878 29.847 0.214 -3.424 -6.341 –
Cavallo et al. 2024 297.88 29.846 0.214 – – –
Hunt & Reffert 2023 297.878 29.847 0.214 -3.424 -6.341 –
Castro-Ginard et al. 2022 297.87 29.84 0.22 -3.41 -6.35 –

💡 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 – – – – – 1516* – –
Cavallo et al. 2024 3.37 2.24 – 132 0.080 – – –
Hunt & Reffert 2023 4.12 2.34 2.38 29 – – – –
Castro-Ginard et al. 2022 4.21 1.70 – 14 – – – –

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

Visualization

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