UBC 392

0.00 UTI

0.48

C_N

1.0

C_dens

0.62

C_C3

0.31

C_lit

0.0

C_dup

C3 classification CA

Number of members (P>50%) 48

Radius (P>50% members) 8.2 [arcmin]

C_N 0.48 Poorly populated
C_dens 1.0 Very dense
C_C3 0.62 Intermediate 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

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UBC 392 is a poorly populated, very dense object of intermediate 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, 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 Young

Data

🔍 Search references for UBC 392 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	–	336.129	64.944	1.06	-0.646	-3.342	-8.82
Alfonso et al.	2024	336.481	65.01	1.039	-0.89	-2.988	–
He et al.	2022	336.726	65.067	1.068	-1.091	-2.889	–
Cantat-Gaudin et al.	2020	336.125	64.926	1.056	-0.642	-3.287	–
Castro-Ginard et al.	2020	336.117	64.931	1.056	-0.643	-3.275	–

💡 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	1.47	–	32	0.011	–	–	–
He et al.	2022	–	2.45	–	13	–	–	–	–
Tarricq et al.	2022	0.94	–	–	85	–	–	–	–
Cantat-Gaudin et al.	2020	0.96	1.47	–	71	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UPK 194	100.0	336.32	64.98	1.06	-0.63	-3.28	-11.95	0.76

💡 Note: The % column shows the percentage of members that UBC 392 shares with each listed object.

Visualization

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