OC 0596

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0.44 UTI
0.32
CN
1.0
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.4 [arcmin]
  • CN 0.32 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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OC 0596 is a poorly populated, very dense object of low 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, 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 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 – 198.851 -61.594 0.574 -6.772 -1.698 –
Hunt & Reffert 2024 198.852 -61.594 0.564 -6.784 -1.672 –
Cavallo et al. 2024 198.851 -61.595 0.568 – – –
Hunt & Reffert 2023 198.852 -61.594 0.564 -6.784 -1.672 –
Hao et al. 2022 198.856 -61.592 0.576 -6.805 -1.67 –

💡 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 – – – – – 233* – –
Cavallo et al. 2024 1.71 2.53 – 178 0.030 – – –
Hunt & Reffert 2023 1.62 1.78 1.99 326 – – – –
Hao et al. 2022 – 4.22 – 398 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 485 93.8 198.85 -61.6 0.58 -6.77 -1.7 – 0.01

💡 Note: The % column shows the percentage of members that OC 0596 shares with each listed object.

Visualization

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