OC 0018

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0.40 UTI
0.0
CN
1.0
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 13.5 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
OC 0018 is a sparse, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.

Palma et al. (2025)
Part of multiple system G49, along with Theia_2045, CWNU_1409 and CWNU_2188.

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 99999– 272.03 -19.406 0.536 0.958 -1.738 -92.274
Hunt & Reffert 2024 272.031 -19.408 0.545 0.912 -1.749 -92.274
Cavallo et al. 2024 272.028 -19.412 0.545 – – –
Hunt & Reffert 2023 272.031 -19.408 0.545 0.912 -1.749 -92.274
Hao et al. 2022 272.027 -19.411 0.538 0.996 -1.704 -2.398

💡 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– 1.56 3.89 2.41 8 0.073 426 – –
Hunt & Reffert 2024 – – – – – 426(1) – –
Cavallo et al. 2024 1.32 3.89 – 26 -0.390 – – –
Hunt & Reffert 2023 1.80 3.39 2.41 8 – – – –
Hao et al. 2022 – 4.85 – 5 0.537 – – –

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

Visualization

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