OC 0557

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0.45 UTI
0.0
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 5.2 [N/pc2]
  • CN 0.0 Sparse
  • 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 0557 is a sparse, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.

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– 163.108 -64.469 0.609 -7.814 2.174 -12.055
Hunt & Reffert 2024 163.072 -64.473 0.613 -7.825 2.176 -10.196
Cavallo et al. 2024 163.088 -64.475 0.617 – – –
Hunt & Reffert 2023 163.072 -64.473 0.613 -7.825 2.176 -10.196
Hao et al. 2022 163.067 -64.48 0.607 -7.618 2.204 –

💡 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– 1.45 1.36 0.34 200 0.075 110 – –
Hunt & Reffert 2024 – – – – – 110(1) – –
Cavallo et al. 2024 1.33 1.36 – 200 -0.460 – – –
Hunt & Reffert 2023 1.57 0.96 0.34 125 – – – –
Hao et al. 2022 – 1.39 – 251 0.611 – – –

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

Visualization

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