CWNU 3092

0.10 UTI

0.42

C_N

0.34

C_dens

0.62

C_C3

0.0

C_lit

0.36

C_dup

C3 classification AC

Number of members (P>50%) 42

Radius (P>50% members) 3.3 [arcmin]

C_N 0.42 Poorly populated
C_dens 0.34 Loose
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.36 Possibly duplicate

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

Overview

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CWNU 3092 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It was recently reported in the literature.

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

Distant Moderate extinction Intermediate age

Data

🔍 Search references for CWNU 3092 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	–	82.199	27.341	0.194	0.257	-1.06	–
He et al.	2023	82.205	27.351	0.194	0.265	-1.071	–

💡 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	3.98	2.35	–	316	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1414	64.3	82.21	27.35	0.2	0.29	-1.06	15.62	0.25

💡 Note: The % column shows the percentage of members that CWNU 3092 shares with each listed object.

Visualization

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