CWNU 3217

0.01 UTI

0.0

C_N

0.86

C_dens

0.25

C_C3

0.0

C_lit

0.04

C_dup

C3 classification DB

Number of members (P>50%) 24

Radius (P>50% members) 2.1 [arcmin]

C_N 0.0 Sparse
C_dens 0.86 Dense
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 0.04 Very likely duplicate

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

Overview

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CWNU 3217 is a sparse, dense object of low C3 quality. Its parallax locates it at a moderate distance, near 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.

Distant High extinction Intermediate age

Data

🔍 Search references for CWNU 3217 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	–	89.492	23.553	0.259	1.135	-0.961	176.127
He et al.	2023	89.491	23.553	0.251	1.13	-0.961	176.13

💡 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	3.24	3.35	–	501	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1473	96.0	89.49	23.55	0.26	1.13	-0.96	176.13	0.22

💡 Note: The % column shows the percentage of members that CWNU 3217 shares with each listed object.

Visualization

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