CWNU 3168

0.12 UTI

0.37

C_N

0.74

C_dens

0.75

C_C3

0.0

C_lit

0.32

C_dup

C3 classification AB

Number of members (P>50%) 37

Radius (P>50% members) 1.3 [arcmin]

C_N 0.37 Poorly populated
C_dens 0.74 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.32 Possibly duplicate

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

Overview

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CWNU 3168 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a large^* distance, well above the mid-plane, affected by moderate extinction. It is catalogued as a young 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.

(*): The parallax distance estimate (~8.35 kpc) differs significantly from the median photometric distance (~5.89 kpc).

Very distant Moderate extinction Young

Data

🔍 Search references for CWNU 3168 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	–	39.846	64.619	0.12	-1.392	0.495	–
He et al.	2023	39.847	64.619	0.127	-1.388	0.494	–

💡 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	5.89	2.85	–	20	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1093	67.6	39.83	64.62	0.13	-1.38	0.5	–	0.4

💡 Note: The % column shows the percentage of members that CWNU 3168 shares with each listed object.

Visualization

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