CWNU 1267

(OCSN 125)

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0.07 UTI
0.0
CN
0.09
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
N50 (P>50% members) 21
Stellar density (N50/rad) 0.4 [N/pc2]
C3 classification DB
  • CN 0.0 Sparse
  • Cdens 0.09 Very loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique
đŸ“Ĩ Members 📊 Colab đŸ”Ŧ Bayestar19 MOCAMOCA 🔍 CDS 🔍 Simbad 🔍 CDS (Îą, δ) 🔍 Simbad (Îą, δ)

Overview
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CWNU 1267 is a sparse, very loose object of low C3 quality. Its parallax locates it at a very close distance, above the mid-plane, affected by low extinction. It is catalogued as a young cluster (see Parameters). It is rarely studied in the literature.

⚠ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Data
🔍 Search references for CWNU 1267 in: SciX Simbad
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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 239.867 -25.659 2.644 -5.514 -4.724 -27.087
Qin et al. 2023 233.57 -29.7 2.6 -6.84 -5.02 -26.38
He et al. 2022 239.648 -25.832 2.656 -5.529 -4.741 –

💡 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– 0.45 0.59 – 84 – – – –
Qin et al. 2023 0.45 0.53 – 89 – – – –
He et al. 2022 – 0.65 – 79 – – – –

Visualization
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CWNU 1267 UCC
Galactocentric position diagram