OC 0492

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0.49 UTI
0.43
CN
1.0
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 6.8 [N/pc2]
  • CN 0.43 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
OC 0492 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a metal-rich, young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature.

Palma et al. (2025)
Part of multiple system G141, along with HSC_2149, UBC_1449 and HSC_2153.

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– 134.263 -46.054 0.45 -4.526 5.484 164.897
Hunt & Reffert 2024 134.282 -46.048 0.456 -4.511 5.486 93.371
Cavallo et al. 2024 134.213 -46.08 0.454 – – –
Hunt & Reffert 2023 134.282 -46.048 0.456 -4.511 5.486 93.371
Hao et al. 2022 134.261 -46.05 0.447 -4.536 5.469 –

💡 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– 2.345 3.42 2.39 25 0.741 519 – –
Hunt & Reffert 2024 – – – – – 519(1) – –
Cavallo et al. 2024 2.56 3.42 – 78 0.870 – – –
Hunt & Reffert 2023 2.13 3.60 2.39 25 – – – –
Hao et al. 2022 – 2.26 – 6 0.611 – – –

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

Visualization

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