UBC 311

0.12 UTI

0.76

C_N

0.92

C_dens

1.0

C_C3

0.0

C_lit

0.23

C_dup

N_m (P>50%) 124

Core radius and density 1.6 [pc], 4.6 [pc^-2]

C3 classification AA

C_N 0.76 Rich
C_dens 0.92 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.23 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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UBC 311 is a rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, below 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 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

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 311 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–	247.195	-54.964	0.712	0.018	-1.259	-3.258
Castro-Ginard et al.	2020	247.205	-54.971	0.692	0.047	-1.271	–

💡 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–	1.3	1.3	–	166	–	–	–	–
Kounkel et al.	2020	1.30	1.30	–	166	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FoF 2210	77.4	247.2	-54.96	0.71	0.02	-1.27	0.09	0.64
CWWDL 3733	58.9	247.18	-54.95	0.71	0.02	-1.25	-3.26	0.0

💡 Note: The % column shows the percentage of members that UBC 311 shares with each listed object.

Visualization

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