UBC 1066

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0.57 UTI
0.57
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.5 [arcmin]
  • CN 0.57 Moderately 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 1066 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Relatively close High 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 – 295.837 22.145 0.378 -3.201 -6.461 –
Hunt & Reffert 2024 295.822 22.146 0.367 -3.176 -6.46 –
Cavallo et al. 2024 295.839 22.143 0.373 – – –
Hunt & Reffert 2023 295.822 22.146 0.367 -3.176 -6.46 –
Castro-Ginard et al. 2022 295.85 22.15 0.37 -3.17 -6.48 –

💡 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 – – – – – 790* – –
Cavallo et al. 2024 2.72 3.69 – 32 0.140 – – –
Hunt & Reffert 2023 2.44 3.50 1.81 27 – – – –
Castro-Ginard et al. 2022 2.77 3.10 – 20 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 412 84.6 295.84 22.14 0.38 -3.2 -6.47 – 0.0

💡 Note: The % column shows the percentage of members that UBC 1066 shares with each listed object.

Visualization

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