UBC 1426

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0.20 UTI
0.3
CN
0.08
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
C3 classification AC
Number of members (P>50%) 30
Radius (P>50% members) 5.8 [arcmin]
  • CN 0.3 Poorly populated
  • Cdens 0.08 Very loose
  • CC3 0.62 Intermediate 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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UBC 1426 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a large 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.

Very distant Low extinction Young

Data
🔍 Search references for UBC 1426 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 – 124.048 -32.982 0.193 -2.661 3.22 –
Castro-Ginard et al. 2022 124.07 -32.97 0.19 -2.65 3.23 –

💡 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
Castro-Ginard et al. 2022 5.75 0.91 – 58 – – – –

Visualization
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UBC 1426 UCC
Galactocentric position diagram