CWNU 1134

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0.32 UTI
0.39
CN
0.45
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 2.2 [N/pc2]
  • CN 0.39 Poorly populated
  • Cdens 0.45 Loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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CWNU 1134 is a poorly populated, loose 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, but with a large variance across recent sources for the absorption and age parameters (see Parameters). It is rarely studied in the literature.

Palma et al. (2025)
Classified as optical pair P293, along with UPK_535.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as moving group. CMD class: 0.91 (50th percentile).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 130.122 -52.891 3.197 -13.702 11.725 19.94
Cavallo et al. 2024 130.851 -53.572 3.194 – – –
Hunt & Reffert 2023 130.252 -52.446 3.188 -13.684 11.757 18.526
He et al. 2022 130.252 -53.81 3.205 -13.954 11.949 –

💡 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– 0.315 0.41 0.43 40 -0.160 – – –
Cavallo et al. 2024 0.32 0.41 – 10 -0.160 – – –
Hunt & Reffert 2023 0.31 0.06 0.43 190 – – – –
He et al. 2022 – 0.50 – 40 – – – –

Visualization

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