OC 0590

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0.25 UTI
0.0
CN
1.0
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 8.3 [arcmin]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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OC 0590 is a sparse, very dense object of low C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, intermediate-age cluster (see Parameters). It is rarely studied in the literature.

Note: This object shares a small percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

Moderate extinction Metal-rich Intermediate age

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 196.615 -59.913 1.498 -11.98 -4.088 -2.682
Hao et al. 2022 196.455 -59.919 1.501 -11.985 -4.132 3.41

💡 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
Hao et al. 2022 – 2.09 – 398 0.611 – – –
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 16.0 195.96 -60.08 1.49 -12.09 -3.87 -2.9 0.0
OC 0588 16.0 195.99 -60.09 1.5 -12.09 -3.88 -2.98 0.54

💡 Note: The % column shows the percentage of members that OC 0590 shares with each listed object.

Visualization

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