UBC 167

0.00 UTI

0.72

C_N

1.0

C_dens

0.75

C_C3

0.31

C_lit

0.0

C_dup

C3 classification AB

Number of members (P>50%) 93

Radius (P>50% members) 8.4 [arcmin]

C_N 0.72 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.31 Poorly studied
C_dup 0.0 Very likely duplicate

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

Overview

ℹ️

UBC 167 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is poorly 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.

Close Moderate extinction Near-solar metallicity Very young

Data

🔍 Search references for UBC 167 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	324.766	62.332	1.087	-2.043	-3.094	-17.91
Li et al.	2025	324.786	62.332	1.065	-2.078	-3.022	–
Alfonso et al.	2024	324.845	62.356	1.053	-2.046	-3.098	–
Celli et al.	2024	324.786	62.332	–	–	–	–
Cantat-Gaudin et al.	2020	324.786	62.332	1.065	-2.078	-3.022	–
Castro-Ginard et al.	2020	324.781	62.373	1.062	-2.073	-3.013	–

💡 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	0.77	1.21	–	13	-0.167	–	–	–
Alfonso et al.	2024	0.93	1.08	–	14	0.010	–	–	–
Celli et al.	2024	–	–	–	22	–	225	–	–
Cantat-Gaudin et al.	2020	0.93	1.08	–	22	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UPK 172	100.0	324.81	62.33	1.09	-2.02	-3.12	-16.97	0.54
UBC 10 a	16.1	324.52	62.1	1.08	-2.11	-3.15	-19.14	0.45

💡 Note: The % column shows the percentage of members that UBC 167 shares with each listed object.

Visualization

ℹ️

1 2