UBC 358

0.06 UTI

0.76

C_N

0.19

C_dens

0.75

C_C3

0.0

C_lit

0.19

C_dup

N_m (P>50%) 115

Core radius and density 4.6 [pc], 0.9 [pc^-2]

C3 classification AB

C_N 0.76 Rich
C_dens 0.19 Very loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.19 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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UBC 358 is a rich, very loose object of 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 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 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 358 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–	283.309	8.129	0.974	-1.316	-3.805	-3.885
Castro-Ginard et al.	2020	283.248	8.111	0.979	-1.339	-3.822	–

💡 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–	0.95	1.39	–	132	–	–	–	–
Kounkel et al.	2020	0.95	1.39	–	132	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UPK 50	80.9	283.31	8.14	0.98	-1.32	-3.81	-3.89	0.51
CWWDL 14442	62.6	283.32	8.18	0.98	-1.32	-3.81	-2.6	0.01

💡 Note: The % column shows the percentage of members that UBC 358 shares with each listed object.

Visualization

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