UBC 1088

0.44 UTI

0.47

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

C3 classification BA

Number of members (P>50%) 47

Radius (P>50% members) 4.7 [arcmin]

C_N 0.47 Poorly populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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UBC 1088 is a poorly populated, very dense object of 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.

Note: This object shares a large percentage of members with 3 later reported entries. See table with shared members information.

Relatively close Moderate extinction Intermediate age

Data

🔍 Search references for UBC 1088 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	–	305.899	31.058	0.55	-2.127	-5.154	4.01
Castro-Ginard et al.	2022	305.89	31.06	0.55	-2.13	-5.17	–

💡 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]	Bfr	BSS
Castro-Ginard et al.	2022	1.92	1.61	–	239	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 30	100.0	305.9	31.06	0.55	-2.13	-5.15	4.01	0.04
Theia 4509	97.9	305.9	31.06	0.55	-2.14	-5.15	4.01	0.02
CWNU 64	48.9	305.9	31.08	0.54	-2.11	-5.15	26.57	0.02

💡 Note: The % column shows the percentage of members that UBC 1088 shares with each listed object.

Visualization

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