OC 0600

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0.54 UTI
0.46
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 13.1 [N/pc2]
  • CN 0.46 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 0600 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the absorption and metallicity parameters (see Parameters). It is poorly studied in the literature.

Palma et al. (2025)
Part of multiple system G161, along with Theia_2651, CWNU_2631 and HSC_2612.

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 99999– 206.968 -63.424 0.325 -6.519 -1.938 -51.801
Hunt & Reffert 2024 206.95 -63.429 0.313 -6.517 -1.965 -34.663
Cavallo et al. 2024 206.998 -63.425 0.317 – – –
Hunt & Reffert 2023 206.95 -63.429 0.313 -6.517 -1.965 -34.663
Hao et al. 2022 206.97 -63.424 0.324 -6.548 -1.947 -51.643

💡 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] Bfrac BSS
UCC 99999– 2.88 3.25 2.93 38 0.336 923 – –
Hunt & Reffert 2024 – – – – – 923(1) – –
Cavallo et al. 2024 2.68 3.25 – 55 0.060 – – –
Hunt & Reffert 2023 3.08 3.37 2.93 38 – – – –
Hao et al. 2022 – 0.94 – 25 0.611 – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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