OC 0189

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0.35 UTI
0.0
CN
1.0
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 5.2 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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OC 0189 is a sparse, very dense object of low C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by high extinction. It is catalogued as a metal-rich, young cluster, but with a large variance across recent sources for the absorption and age parameters (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.

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 99999– 336.299 62.313 0.554 -4.126 -3.878 –
Hunt & Reffert 2024 336.291 62.327 0.552 -4.128 -3.913 –
Cavallo et al. 2024 336.3 62.312 0.555 – – –
Hunt & Reffert 2023 336.291 62.327 0.552 -4.128 -3.913 –
Hao et al. 2022 336.276 62.309 0.556 -4.154 -3.835 –

💡 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] Bfrac BSS
UCC 99999– 1.94 3.41 2.62 71 0.571 214 – –
Hunt & Reffert 2024 – – – – – 214(1) – –
Cavallo et al. 2024 2.19 3.41 – 71 0.530 – – –
Hunt & Reffert 2023 1.69 3.56 2.62 255 – – – –
Hao et al. 2022 – 0.46 – 8 0.611 – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 505 96.0 336.31 62.33 0.55 -4.15 -3.87 11.96 0.08

💡 Note: The % column shows the percentage of members that OC 0189 shares with each listed object.

Visualization

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