UBC 1333

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0.56 UTI
0.32
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 1.8 [arcmin]
  • CN 0.32 Poorly 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 1333 is a poorly 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 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.

Distant Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 102.329 3.985 0.244 -0.497 -0.149 –
Hunt & Reffert 2024 102.327 3.986 0.243 -0.473 -0.16 –
Cavallo et al. 2024 102.335 3.969 0.246 – – –
Hunt & Reffert 2023 102.327 3.986 0.243 -0.473 -0.16 –
Castro-Ginard et al. 2022 102.32 3.98 0.24 -0.49 -0.16 –

💡 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 – – – – – 313* – –
Cavallo et al. 2024 3.31 1.00 – 162 0.330 – – –
Hunt & Reffert 2023 3.56 1.50 2.04 51 – – – –
Castro-Ginard et al. 2022 4.67 1.52 – 5 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 266 96.9 102.33 3.99 0.24 -0.5 -0.15 – 0.01

💡 Note: The % column shows the percentage of members that UBC 1333 shares with each listed object.

Visualization

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