UBC 116

0.01 UTI

0.63

C_N

0.45

C_dens

0.75

C_C3

0.0

C_lit

0.04

C_dup

N_m (P>50%) 76

Core radius and density 1.6 [pc], 2.3 [pc^-2]

C3 classification AB

C_N 0.63 Moderately populated
C_dens 0.45 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.04 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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UBC 116 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a young 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.

Close Moderate extinction Young

Castro-Ginard et al. (2020)
Coincidence with Sim et al. (2019, J. Korean Astron. Soc., 52, 145) or Liu & Pang (2019ApJS..245...32L), see Sect. 4.1.5.

Data

🔍 Search references for UBC 116 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–	291.699	0.2	1.125	-0.623	-2.15	4.191
Castro-Ginard et al.	2020	291.679	0.199	1.103	-0.707	-2.099	–

💡 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–	0.86	1.02	–	85	–	–	–	–
Kounkel et al.	2020	0.86	1.02	–	85	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UPK 45	96.1	291.71	0.2	1.13	-0.62	-2.16	4.11	0.6
CWWDL 14314	63.2	291.7	0.22	1.13	-0.65	-2.15	4.58	0.0

💡 Note: The % column shows the percentage of members that UBC 116 shares with each listed object.

Visualization

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