CWNU 1015

(OCSN 164)

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0.44 UTI
0.45
CN
0.52
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 2.6 [N/pc2]
  • CN 0.45 Poorly populated
  • Cdens 0.52 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1015 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a very close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.

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– 75.847 -3.368 5.729 11.954 -14.235 25.664
Cavallo et al. 2024 73.67 -1.252 5.775 – – –
Hunt & Reffert 2023 76.544 -3.338 5.766 12.775 -15.57 24.188
Qin et al. 2023 75.89 -3.1 5.93 11.64 -14.6 23.8
He et al. 2022 75.331 -3.707 5.72 12.055 -14.383 –

💡 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– 0.17 0.305 0.65 45 0.160 – – –
Cavallo et al. 2024 0.17 0.59 – 40 0.160 – – –
Hunt & Reffert 2023 0.17 0.16 0.65 34 – – – –
Qin et al. 2023 0.18 0.12 – 79 – – – –
He et al. 2022 – 0.45 – 50 – – – –

Visualization

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