DBSB 167

(DBS2003 167; MWSC 2394)

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0.18 UTI
0.0
CN
0.15
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
N50 (P>50% members) 17
Stellar density (N50/rad) 0.8 [N/pc2]
C3 classification CC
  • CN 0.0 Sparse
  • Cdens 0.15 Very loose
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly 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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DBSB 167 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a very young cluster (see Parameters). It is poorly 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.

Morales et al. (2013)
Classified as morphological type 'OC0' (emerging exposed cluster). Morphological flag: possibly associated submm emission surrounding the cluster.

Data
🔍 Search references for DBSB 167 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– 245.77 -49.475 0.271 -3.758 -3.65 -47.864
Just et al. 2023 245.847 -49.544 – – – –
Kharchenko et al. 2016 245.847 -49.544 – – – –
Kharchenko et al. 2013 245.857 -49.545 – -5.61 2.95 –
Morales et al. 2013 245.85 -49.541 – – – –

💡 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– 4.08 4.32 – 2 – 198 – –
Just et al. 2023 – – – 2 – 198 – –
Kharchenko et al. 2016 4.08 4.32 – 2 – – – –
Kharchenko et al. 2013 4.08 4.32 – 2 – – – –
Morales et al. 2013 10.21 – – – – – – –

Visualization
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DBSB 167 UCC
Galactocentric position diagram