DBSB 60

(DBSB2003 60; MWSC 1888)

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0.22 UTI
0.0
CN
0.04
Cdens
0.62
CC3
0.23
Clit
1.0
Cdup
Nm (P>50%) 18
Core radius and density 5.3 [pc], 0.2 [pc-2]
C3 classification AC
  • CN 0.0 Sparse
  • Cdens 0.04 Very loose
  • CC3 0.62 Intermediate quality
  • Clit 0.23 Rarely studied
  • Cdup 1.0 Unique
đŸ“Ĩ Members 📊 Colab đŸ”Ŧ Bayestar19 MOCAMOCA 🔍 CDS 🔍 Simbad 🔍 CDS (Îą, δ) 🔍 Simbad (Îą, δ)

Overview
ℹī¸
DBSB 60 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by high extinction. It is catalogued as a very 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.

Dutra et al. (2003)
Classified as infrared cluster (IRC).

Data
🔍 Search references for DBSB 60 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– 166.355 -62.476 0.178 -5.269 1.854 34.157
Celli et al. 2024 166.385 -62.482 – – – –
Just et al. 2023 166.396 -62.482 – – – –
Cantat-Gaudin et al. 2020 166.385 -62.482 0.202 -5.229 1.874 –
Cantat-Gaudin & Anders 2020 166.385 -62.482 0.202 -5.229 1.874 –
Cantat-Gaudin et al. 2018 166.385 -62.482 0.202 -5.229 1.874 –
Kharchenko et al. 2016 166.396 -62.482 – – – –
Kharchenko et al. 2013 166.404 -62.485 – -10.49 4.76 –
Dutra et al. 2003 166.411 -62.486 – – – –

💡 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– 4.05 4.27 – 6 – 251 – –
Celli et al. 2024 – – – 6 – 252 – –
Just et al. 2023 – – – 6 – 250 – –
Kounkel et al. 2020 4.05 4.06 – 10 – – – –
Cantat-Gaudin & Anders 2020 4.32 – – – – – – –
Cantat-Gaudin et al. 2018 4.32 – – – – – – –
Kharchenko et al. 2016 3.74 4.27 – 6 – – – –
Kharchenko et al. 2013 3.74 4.27 – 6 – – – –

Visualization
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DBSB 60 UCC
DBSB 60 CANTAT20
Galactocentric position diagram