CWNU 1262

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0.27 UTI
0.26
CN
0.32
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 1.6 [N/pc2]
  • CN 0.26 Poorly populated
  • Cdens 0.32 Loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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CWNU 1262 is a poorly populated, loose 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, very young cluster (see Parameters). It is rarely 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– 73.296 -10.756 3.556 -0.45 -1.403 5.275
Cavallo et al. 2024 73.012 -10.646 3.552 – – –
Hunt & Reffert 2023 73.157 -10.55 3.559 -0.397 -1.377 9.81
He et al. 2022 73.235 -10.733 3.566 -0.42 -1.574 –

💡 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– 0.28 0.42 0.69 18 -0.350 – – –
Cavallo et al. 2024 0.28 0.94 – 10 -0.350 – – –
Hunt & Reffert 2023 0.28 0.42 0.69 18 – – – –
He et al. 2022 – 0.20 – 22 – – – –

Visualization

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