UBC 267

0.14 UTI

0.52

C_N

0.63

C_dens

0.75

C_C3

0.31

C_lit

0.28

C_dup

C3 classification AB

Number of members (P>50%) 54

Radius (P>50% members) 4.6 [arcmin]

C_N 0.52 Moderately populated
C_dens 0.63 Moderately dense
C_C3 0.75 High quality
C_lit 0.31 Poorly studied
C_dup 0.28 Possibly duplicate

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

Overview

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UBC 267 is a moderately populated, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is poorly studied in the literature.

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

Relatively close Low extinction Near-solar metallicity Very young

Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit.

Data

🔍 Search references for UBC 267 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	–	168.345	-58.936	0.323	-6.016	1.831	–
Almeida et al.	2025	168.3	-58.906	–	–	–	–
Celli et al.	2024	168.283	-58.901	–	–	–	–
Dias et al.	2021	168.3	-58.906	0.305	-6.011	1.817	–
Cantat-Gaudin et al.	2020	168.283	-58.901	0.311	-6.016	1.809	–
Castro-Ginard et al.	2020	168.305	-58.883	0.309	-6.013	1.823	–

💡 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
Almeida et al.	2025	2.88	0.91	–	7	–	925	–	–
Celli et al.	2024	–	–	–	13	–	695	–	–
Dias et al.	2021	2.88	0.91	–	7	0.200	–	–	–
Cantat-Gaudin et al.	2020	2.42	0.46	–	13	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Stock 13	72.2	168.29	-58.89	0.33	-6.03	1.9	-13.12	0.78

💡 Note: The % column shows the percentage of members that UBC 267 shares with each listed object.

Visualization

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