UBC 250

0.05 UTI

0.58

C_N

0.44

C_dens

0.75

C_C3

0.31

C_lit

0.1

C_dup

C3 classification AB

Number of members (P>50%) 67

Radius (P>50% members) 20.1 [arcmin]

C_N 0.58 Moderately populated
C_dens 0.44 Loose
C_C3 0.75 High quality
C_lit 0.31 Poorly studied
C_dup 0.1 Likely duplicate

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

Overview

ℹ️

UBC 250 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

⚠️ Warning: This is 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 Low extinction Near-solar metallicity Intermediate age

Data

🔍 Search references for UBC 250 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	118.177	-60.357	1.055	-3.494	10.953	14.536
Alfonso et al.	2024	118.765	-60.244	1.017	-3.581	10.946	–
He et al.	2022	118.114	-60.37	1.055	-3.483	10.973	–
Tarricq et al.	2022	118.11	-60.369	1.06	-3.462	10.96	–
Cantat-Gaudin et al.	2020	118.12	-60.373	1.016	-3.502	10.888	–
Castro-Ginard et al.	2020	118.169	-60.368	1.022	-3.465	10.926	–

💡 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
Alfonso et al.	2024	0.96	0.31	–	549	0.010	–	–	–
He et al.	2022	–	0.55	–	355	–	–	–	–
Tarricq et al.	2022	0.94	–	–	347	–	–	–	–
Cantat-Gaudin et al.	2020	0.96	0.31	–	331	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
ESO 123 26	89.6	118.19	-60.3	1.06	-3.5	10.97	14.54	0.7

💡 Note: The % column shows the percentage of members that UBC 250 shares with each listed object.

Visualization

ℹ️

1 2