UBC 223

0.00 UTI

0.78

C_N

0.45

C_dens

0.75

C_C3

0.0

C_lit

0.0

C_dup

N_m (P>50%) 184

Core radius and density 2.6 [pc], 2.2 [pc^-2]

C3 classification AB

C_N 0.78 Rich
C_dens 0.45 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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UBC 223 is a rich, loose object of high C3 quality. Its parallax locates it at a moderate distance, near 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, and a large percentage with at least one entry reported in the same catalogue. See table with shared members information.

Distant 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 223 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–	112.123	-20.114	0.286	-2.255	2.525	67.724
Castro-Ginard et al.	2020	112.116	-20.112	0.266	-2.269	2.549	–

💡 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–	3.23	1.48	–	71	–	–	–	–
Kounkel et al.	2020	3.23	1.48	–	71	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FoF 198	99.5	112.12	-20.12	0.29	-2.25	2.51	67.72	0.49
UBC 635	79.3	112.12	-20.13	0.32	-2.23	2.48	67.72	0.05

💡 Note: The % column shows the percentage of members that UBC 223 shares with each listed object.

Visualization

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