CWNU 3096

0.03 UTI

0.51

C_N

1.0

C_dens

0.5

C_C3

0.0

C_lit

0.08

C_dup

C3 classification BB

Number of members (P>50%) 52

Radius (P>50% members) 1.4 [arcmin]

C_N 0.51 Moderately populated
C_dens 1.0 Very dense
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.08 Very likely duplicate

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

Overview

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CWNU 3096 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as an old cluster (see Parameters). It was recently reported 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 Old

Data

🔍 Search references for CWNU 3096 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	–	101.661	-2.097	0.206	-0.306	-0.296	83.286
He et al.	2023	101.659	-2.095	0.216	-0.305	-0.314	86.76

💡 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
He et al.	2023	4.37	2.50	–	1259	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1690	92.3	101.66	-2.1	0.22	-0.35	-0.27	83.29	0.46

💡 Note: The % column shows the percentage of members that CWNU 3096 shares with each listed object.

Visualization

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