CWNU 4860

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0.03 UTI
0.0
CN
0.03
Cdens
0.12
CC3
0.0
Clit
1.0
Cdup
C3 classification DC
Number of members (P>50%) 15
Radius (P>50% members) 3.7 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.03 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique
đŸ“Ĩ Members 📊 Colab đŸ”Ŧ Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (Îą, δ) 🔍 Simbad (Îą, δ)

Overview
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CWNU 4860 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large distance, well below the mid-plane, affected by low extinction. It is catalogued as a very old cluster (see Parameters). It was recently reported 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.

Very distant Low extinction Very old

Data
🔍 Search references for CWNU 4860 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 – 155.064 -63.706 0.116 -4.764 2.966 4.458
He et al. 2023 155.042 -63.721 0.166 -4.764 3.0 14.08

💡 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] Bfr BSS
He et al. 2023 9.33 0.20 – 7943 – – – –

Visualization
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CWNU 4860 UCC
Galactocentric position diagram