UBC 1622

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0.48 UTI
0.0
CN
1.0
Cdens
0.75
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 2.7 [arcmin]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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UBC 1622 is a sparse, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age 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 Low extinction Near-solar metallicity Intermediate age

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 – 147.599 -48.206 0.39 -6.064 4.367 3.858
Hu & Soubiran 2025 147.59 -48.212 – – – –
Hunt & Reffert 2024 147.599 -48.218 0.384 -6.053 4.375 3.677
Cavallo et al. 2024 147.59 -48.212 0.384 – – –
Hunt & Reffert 2023 147.599 -48.218 0.384 -6.053 4.375 3.677
Castro-Ginard et al. 2022 147.59 -48.22 0.38 -6.07 4.35 4.42

💡 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
Hu & Soubiran 2025 – – – – -0.260* – – –
Hunt & Reffert 2024 – – – – – 148* – –
Cavallo et al. 2024 2.25 0.70 – 603 -0.050 – – –
Hunt & Reffert 2023 2.38 0.29 0.81 728 – – – –
Castro-Ginard et al. 2022 2.96 0.48 – 410 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 12626 76.0 147.58 -48.2 0.38 -6.09 4.37 3.79 0.08

💡 Note: The % column shows the percentage of members that UBC 1622 shares with each listed object.

Visualization

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