UBC 1060

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0.63 UTI
0.63
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.9 [arcmin]
  • CN 0.63 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 1060 is a moderately populated, very dense object of very 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 – 292.96 16.543 0.459 -1.103 -3.585 127.728
Hunt & Reffert 2024 292.972 16.539 0.447 -1.11 -3.571 127.739
Cavallo et al. 2024 292.966 16.56 0.449 – – –
Hunt & Reffert 2023 292.972 16.539 0.447 -1.11 -3.571 127.739
Castro-Ginard et al. 2022 292.97 16.56 0.47 -1.1 -3.6 –

💡 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 – – – – – 724* – –
Cavallo et al. 2024 2.40 3.67 – 10 0.460 – – –
Hunt & Reffert 2023 2.05 3.60 1.49 27 – – – –
Castro-Ginard et al. 2022 2.47 3.20 – 47 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 122 98.7 292.96 16.54 0.46 -1.1 -3.58 127.73 0.03

💡 Note: The % column shows the percentage of members that UBC 1060 shares with each listed object.

Visualization

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