DBSB 80

(MWSC 2068)

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0.42 UTI
0.34
CN
1.0
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
C3 classification AB
Number of members (P>50%) 34
Radius (P>50% members) 0.8 [arcmin]
  • CN 0.34 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High 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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DBSB 80 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by high extinction. It is catalogued as a low-mass, very young cluster (see Parameters). It is rarely studied in the literature.
Relatively close High extinction Low mass Very young

Data
🔍 Search references for DBSB 80 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 – 192.593 -61.582 0.558 -6.74 -2.416 –
Just et al. 2023 192.584 -61.578 – – – –
Kharchenko et al. 2016 192.584 -61.578 – – – –
Kharchenko et al. 2013 192.595 -61.582 – -11.53 0.82 -17.0

💡 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
Just et al. 2023 – – – 8 – 26 – –
Kharchenko et al. 2016 2.13 4.39 – 8 – – – –
Kharchenko et al. 2013 2.13 4.39 – 8 – – – –

Visualization
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DBSB 80 UCC
Galactocentric position diagram