CWNU 1138

(OCSN 179)

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0.56 UTI
0.56
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 5.4 [N/pc2]
  • CN 0.56 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1138 is a moderately populated, very dense object of 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 (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– 206.552 -59.475 2.015 -13.837 -6.15 -20.197
Cavallo et al. 2024 206.633 -59.511 2.015 – – –
Hunt & Reffert 2023 206.912 -59.633 2.012 -13.866 -6.156 -20.586
Qin et al. 2023 206.64 -59.47 2.01 -13.76 -6.11 -21.65
He et al. 2022 206.624 -59.559 2.013 -13.828 -6.095 –

💡 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– 0.49 0.74 1.11 84 -0.040 – – –
Cavallo et al. 2024 0.49 0.78 – 87 -0.040 – – –
Hunt & Reffert 2023 0.48 0.47 1.11 82 – – – –
Qin et al. 2023 0.69 0.81 – 178 – – – –
He et al. 2022 – 0.70 – 63 – – – –

Visualization

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