UBC 196

0.03 UTI

0.8

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.05

C_dup

N_m (P>50%) 237

Core radius and density 1.4 [pc], 8.6 [pc^-2]

C3 classification AA

C_N 0.8 Rich
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.05 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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UBC 196 is a rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 6 years.

⚠️ 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 Intermediate age

Data

🔍 Search references for UBC 196 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	99999–	90.664	49.88	0.757	0.815	-2.599	-13.21
Castro-Ginard et al.	2020	90.668	49.893	0.754	0.873	-2.614	–

💡 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]	B_frac	BSS
UCC	99999–	1.21	1.31	–	851	–	–	–	–
Kounkel et al.	2020	1.21	1.31	–	851	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
NGC 2126	94.9	90.66	49.88	0.76	0.81	-2.6	-12.89	0.96

💡 Note: The % column shows the percentage of members that UBC 196 shares with each listed object.

Visualization

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