UBC 1079

0.02 UTI

0.45

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.04

C_dup

N₅₀ (P>50% members) 45

Stellar density (N₅₀/rad) 9.6 [N/pc²]

C3 classification AB

C_N 0.45 Poorly populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.04 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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UBC 1079 is a poorly populated, very 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 an intermediate-age 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.

Relatively close Moderate extinction Intermediate age

Data

🔍 Search references for UBC 1079 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–	298.319	32.66	0.482	-2.484	-3.446	10.049
Castro-Ginard et al.	2022	298.33	32.67	0.49	-2.48	-3.45	–

💡 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–	2.21	1.36	–	141	–	–	–	–
Castro-Ginard et al.	2022	2.21	1.36	–	141	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HXHWL 46	95.6	298.31	32.65	0.47	-2.48	-3.44	10.05	0.56
CWWDL 11597	73.3	298.3	32.65	0.47	-2.46	-3.46	-1.29	0.06
CWWDL 14020	62.2	298.3	32.63	0.47	-2.46	-3.45	10.05	0.03

💡 Note: The % column shows the percentage of members that UBC 1079 shares with each listed object.

Visualization

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