UBC 1089

0.03 UTI

0.45

C_N

0.73

C_dens

0.75

C_C3

0.0

C_lit

0.07

C_dup

C3 classification BA

Number of members (P>50%) 45

Radius (P>50% members) 4.3 [arcmin]

C_N 0.45 Poorly populated
C_dens 0.73 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.07 Very likely duplicate

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

Overview

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UBC 1089 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a young cluster (see Parameters). It is rarely studied in the literature.

⚠️ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Distant Moderate extinction Young

Data

🔍 Search references for UBC 1089 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	–	301.193	33.961	0.357	-1.998	-5.54	11.22
Castro-Ginard et al.	2022	301.2	33.95	0.35	-1.99	-5.56	–

💡 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	3.02	1.73	–	80	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Berkeley 84	93.3	301.2	33.95	0.36	-2.01	-5.55	11.22	0.63

💡 Note: The % column shows the percentage of members that UBC 1089 shares with each listed object.

Visualization

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