CWNU 122

0.03 UTI

0.65

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.06

C_dup

N₅₀ (P>50% members) 80

Stellar density (N₅₀/rad) 13.9 [N/pc²]

C3 classification AA

C_N 0.65 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.06 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 122 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, 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.

Relatively close High extinction Near-solar metallicity Young

Data

🔍 Search references for CWNU 122 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–	292.964	16.541	0.461	-1.103	-3.583	127.728
He et al.	2022	292.969	16.54	0.46	-1.11	-3.58	–

💡 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–	1.82	3.84	–	25	0.274	–	–	–
He et al.	2022	1.82	3.84	–	25	0.274	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1060	93.8	292.96	16.54	0.46	-1.1	-3.58	127.73	0.63

💡 Note: The % column shows the percentage of members that CWNU 122 shares with each listed object.

Visualization

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