CWNU 1124

0.03 UTI

0.0

C_N

0.06

C_dens

0.12

C_C3

0.0

C_lit

0.8

C_dup

N₅₀ (P>50% members) 21

Radius (P>50% members) 78.6 [arcmin]

C3 classification DC

C_N 0.0 Sparse
C_dens 0.06 Very loose
C_C3 0.12 Very low quality
C_lit 0.0 Rarely studied
C_dup 0.8 Very likely unique

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

Overview

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CWNU 1124 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a young cluster (see Parameters). It is rarely studied in the literature.

Note: This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry. See table with shared members information.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=0.8) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Low extinction Young

Data

🔍 Search references for CWNU 1124 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–	324.767	50.258	2.83	7.142	1.765	-16.919
He et al.	2022	324.639	50.397	2.855	7.069	1.839	–

💡 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–	–	0.35	–	56	–	–	–	–
He et al.	2022	–	0.35	–	56	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
NGC 7058	20.0	320.47	50.82	2.73	7.45	2.75	-19.44	1.0

💡 Note: The % column shows the percentage of members that CWNU 1124 shares with each listed object.

Visualization

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