OC 0588

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0.54 UTI
0.44
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 10.8 [arcmin]
  • CN 0.44 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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OC 0588 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a close 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 very small percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

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 – 195.99 -60.087 1.496 -12.09 -3.88 -2.979
Hunt & Reffert 2024 195.998 -60.096 1.497 -12.071 -3.854 -2.313
Cavallo et al. 2024 195.798 -59.93 1.499 – – –
Hunt & Reffert 2023 195.998 -60.096 1.497 -12.071 -3.854 -2.313
Hao et al. 2022 195.992 -60.09 1.489 -12.054 -3.868 -1.106

💡 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 – – – – – 623* – –
Cavallo et al. 2024 0.66 0.82 – 316 0.300 – – –
Hunt & Reffert 2023 0.63 0.64 0.89 232 – – – –
Hao et al. 2022 – 2.45 – 631 0.112 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1122 100.0 196.04 -59.99 1.5 -12.07 -3.91 -2.83 0.42
CWWDL 14425 84.1 195.96 -60.08 1.49 -12.09 -3.87 -2.9 0.0
OC 0590 9.1 196.62 -59.91 1.5 -11.98 -4.09 -2.68 0.25

💡 Note: The % column shows the percentage of members that OC 0588 shares with each listed object.

Visualization

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