CWNU 515

(OCSN 157)

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0.63 UTI
0.34
CN
1.0
Cdens
1.0
CC3
0.4
Clit
1.0
Cdup
Stellar density (N50/rad) 6.0 [N/pc2]
  • CN 0.34 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.4 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 515 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low 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.

Liu et al. (2025)
Classified as tidal capture (resonant trapping binary) 79 along with HSC_2351.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 131.812 -63.409 4.859 -26.564 15.495 11.108
Wei et al. 2025 131.962 -63.136 4.859 -26.769 15.395 –
Cavallo et al. 2024 133.149 -63.402 4.867 – – –
Hunt & Reffert 2023 131.902 -63.583 4.869 -27.101 14.774 8.118
Qin et al. 2023 131.9 -63.43 4.87 -26.77 15.43 11.13
He et al. 2022 131.893 -63.346 4.862 -26.528 15.418 –
He et al. 2022 132.183 -63.529 4.84 -26.65 15.39 11.9

💡 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– 0.21 0.31 0.5 28 -0.250 56 0.51 –
Liu et al. 2025 0.21 0.07 – 35 – – – –
Wei et al. 2025 0.22 0.40 – 27 -0.250 56 0.51 –
Cavallo et al. 2024 0.20 0.63 – 32 0.100 – – –
Hunt & Reffert 2023 0.21 0.12 0.50 21 – – – –
Qin et al. 2023 0.23 0.31 – 28 – – – –
He et al. 2022 – 0.20 – 32 – – – –
He et al. 2022 0.21 0.42 – 25 -0.419 – – –

Visualization

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