DBSB 60

(MWSC 1888)

0.33 UTI

0.0

C_N

0.16

C_dens

0.62

C_C3

0.44

C_lit

1.0

C_dup

C3 classification AC

Number of members (P>50%) 18

Radius (P>50% members) 2.9 [arcmin]

C_N 0.0 Sparse
C_dens 0.16 Very loose
C_C3 0.62 Intermediate quality
C_lit 0.44 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

ℹ️

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 poorly studied in the literature.

(*): The parallax distance estimate (~5.61 kpc) differs significantly from the median photometric distance (~4.03 kpc).

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Distant High extinction Very young

Data

🔍 Search references for DBSB 60 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	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	–

💡 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
Celli et al.	2024	–	–	–	6	–	252	–	–
Just et al.	2023	–	–	–	6	–	250	–	–
Cantat-Gaudin & Anders	2020	4.32	–	–	–	–	–	–	–
Cantat-Gaudin et al.	2018	4.32	–	–	–	–	–	–	–
Kharchenko et al.	2016	3.74	4.19	–	6	–	–	–	–
Kharchenko et al.	2013	3.74	4.19	–	6	–	–	–	–

Visualization

ℹ️

1 2