CWNU 3165

0.03 UTI

0.56

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%) 62

Radius (P>50% members) 2.2 [arcmin]

C_N 0.56 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 3165 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as an intermediate-age 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.

Relatively close High extinction Intermediate age

Data

🔍 Search references for CWNU 3165 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	–	304.508	39.72	0.276	-3.808	-6.362	-12.459
He et al.	2023	304.507	39.723	0.276	-3.813	-6.36	–

💡 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	2.95	4.05	–	251	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Teutsch 139	91.9	304.51	39.72	0.28	-3.81	-6.36	-11.17	0.41
HSC 608	80.6	304.51	39.72	0.27	-3.8	-6.36	-11.17	0.01

💡 Note: The % column shows the percentage of members that CWNU 3165 shares with each listed object.

Visualization

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