DBSB 10

(MWSC 1272)

Click to load Aladin Lite
0.33 UTI
0.28
CN
1.0
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
C3 classification BC
Number of members (P>50%) 28
Radius (P>50% members) 2.3 [arcmin]
  • CN 0.28 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.38 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
ℹī¸
DBSB 10 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a very young cluster (see Parameters). It is rarely studied in the literature.
Relatively close Moderate extinction Very young

Data
🔍 Search references for DBSB 10 in: SciX Simbad
ℹī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 113.869 -22.398 0.388 -2.434 2.079 95.6
Just et al. 2023 113.851 -22.392 – – – –
Kharchenko et al. 2016 113.851 -22.392 – – – –
Kharchenko et al. 2013 113.857 -22.395 – -5.2 1.33 –

💡 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 – – – 3 – 197 – –
Kharchenko et al. 2016 2.36 1.29 – 3 – – – –
Kharchenko et al. 2013 2.36 1.29 – 3 – – – –

Visualization
ℹī¸
DBSB 10 UCC
Galactocentric position diagram