OC 0192

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0.43 UTI
0.0
CN
1.0
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 9.6 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
OC 0192 is a sparse, very dense object of intermediate C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, 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 G261, along with Theia_1001 and CWNU_58.

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– 343.388 57.529 1.085 -0.732 -1.538 -15.174
Hunt & Reffert 2024 343.388 57.524 1.067 -0.75 -1.485 -17.361
Cavallo et al. 2024 343.642 57.581 1.067 – – –
Hunt & Reffert 2023 343.388 57.524 1.067 -0.75 -1.485 -17.361
Hao et al. 2022 343.411 57.537 1.103 -0.679 -1.659 –

💡 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– 0.92 1.27 0.31 50 -0.179 68 – –
Hunt & Reffert 2024 – – – – – 68(1) – –
Cavallo et al. 2024 0.94 1.48 – 21 -0.470 – – –
Hunt & Reffert 2023 0.90 0.71 0.31 72 – – – –
Hao et al. 2022 – 1.27 – 50 0.112 – – –

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

Visualization

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