UBC 1189

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0.53 UTI
0.38
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.0 [arcmin]
  • CN 0.38 Poorly 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 1189 is a poorly populated, very dense object of 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, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a large percentage of members with 2 later reported entries. See table with shared members information.

Relatively close Moderate 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 – 356.063 62.675 0.368 -3.842 -1.92 –
Hunt & Reffert 2024 356.059 62.672 0.359 -3.84 -1.925 –
Cavallo et al. 2024 356.094 62.662 0.362 – – –
Hunt & Reffert 2023 356.059 62.672 0.359 -3.84 -1.925 –
Castro-Ginard et al. 2022 356.05 62.66 0.37 -3.85 -1.92 –

💡 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 – – – – – 366* – –
Cavallo et al. 2024 2.64 2.32 – 158 0.240 – – –
Hunt & Reffert 2023 2.55 2.17 1.23 131 – – – –
Castro-Ginard et al. 2022 2.89 2.06 – 127 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 219 89.5 356.06 62.67 0.37 -3.84 -1.92 – 0.02
CWWDL 2585 2.6 356.0 62.66 0.33 -3.68 -1.47 -65.43 0.25

💡 Note: The % column shows the percentage of members that UBC 1189 shares with each listed object.

Visualization

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