OC 0589

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0.36 UTI
0.39
CN
0.41
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 7.8 [arcmin]
  • CN 0.39 Poorly populated
  • Cdens 0.41 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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OC 0589 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Very 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 – 196.275 -61.722 0.518 -4.949 -1.593 –
Hunt & Reffert 2024 196.225 -61.707 0.52 -4.947 -1.573 17.386
Cavallo et al. 2024 196.881 -61.419 0.52 – – –
Hunt & Reffert 2023 196.225 -61.707 0.52 -4.947 -1.573 17.386
Hao et al. 2022 196.423 -61.712 0.535 -4.997 -1.581 –

💡 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 – – – – – 246* – –
Cavallo et al. 2024 2.06 2.50 – 17 0.370 – – –
Hunt & Reffert 2023 1.83 2.03 2.67 21 – – – –
Hao et al. 2022 – 2.28 – 5 0.611 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 467 56.4 196.36 -61.74 0.51 -4.99 -1.64 – 0.09

💡 Note: The % column shows the percentage of members that OC 0589 shares with each listed object.

Visualization

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