UBC 1465

0.49 UTI

0.75

C_N

0.95

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 109

Stellar density (N₅₀/rad) 4.8 [N/pc²]

C3 classification AB

C_N 0.75 Rich
C_dens 0.95 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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UBC 1465 is a rich, very dense 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.

Note: This object shares a significant percentage of members with 4 later reported entries. See table with shared members information.

Relatively close Moderate extinction Intermediate age

Data

🔍 Search references for UBC 1465 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–	146.893	-50.574	0.638	-7.155	5.004	20.527
Castro-Ginard et al.	2022	146.87	-50.56	0.65	-7.16	5.0	–

💡 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–	1.72	1.33	–	169	–	–	–	–
Castro-Ginard et al.	2022	1.72	1.33	–	169	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv
Theia 6111	72.5	146.9	-50.57	0.64	-7.15	5.0	18.59
CWNU 184	59.6	146.87	-50.56	0.64	-7.14	5.01	13.24
CWWDL 14184	53.2	146.87	-50.55	0.65	-7.14	5.01	18.79
CWWDL 13969	36.7	146.87	-50.54	0.64	-7.15	5.03	20.92

💡 Note: The % column shows the percentage of members that UBC 1465 shares with each listed object.

Visualization

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