UBC 667

0.01 UTI

0.47

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.02

C_dup

C3 classification AA

Number of members (P>50%) 47

Radius (P>50% members) 1.2 [arcmin]

C_N 0.47 Poorly populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.02 Very likely duplicate

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

Overview

ℹ️

UBC 667 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is rarely studied in the literature.

⚠️ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Intermediate age

Data

🔍 Search references for UBC 667 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	247.738	-48.389	0.345	-1.714	-3.471	–
Li et al.	2025	247.745	-48.386	0.326	-1.679	-3.5	–
Cantat-Gaudin et al.	2020	247.745	-48.386	0.326	-1.679	-3.5	–
Castro-Ginard et al.	2020	247.744	-48.392	0.327	-1.702	-3.48	–

💡 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
Li et al.	2025	2.05	2.27	–	246	-0.040	–	–	–
Cantat-Gaudin et al.	2020	2.90	2.21	–	34	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Teutsch 82	97.9	247.74	-48.39	0.36	-1.73	-3.47	–	0.62

💡 Note: The % column shows the percentage of members that UBC 667 shares with each listed object.

Visualization

ℹ️

1 2