OC 0587

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0.50 UTI
0.4
CN
1.0
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.6 [arcmin]
  • CN 0.4 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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OC 0587 is a poorly populated, very dense object of intermediate 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 (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 High extinction Metal-rich 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 – 193.709 -61.767 0.523 -5.246 -1.345 97.644
Hunt & Reffert 2024 193.707 -61.767 0.517 -5.285 -1.339 61.871
Cavallo et al. 2024 193.661 -61.771 0.517 – – –
Hunt & Reffert 2023 193.707 -61.767 0.517 -5.285 -1.339 61.871
Hao et al. 2022 193.709 -61.762 0.547 -5.199 -1.33 –

💡 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 – – – – – 722* – –
Cavallo et al. 2024 1.98 3.20 – 56 0.440 – – –
Hunt & Reffert 2023 1.84 3.51 2.45 31 – – – –
Hao et al. 2022 – 1.99 – 8 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 486 100.0 193.68 -61.76 0.51 -5.26 -1.35 84.84 0.3

💡 Note: The % column shows the percentage of members that OC 0587 shares with each listed object.

Visualization

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