CWNU 3215

0.18 UTI

0.6

C_N

0.46

C_dens

0.5

C_C3

0.0

C_lit

0.57

C_dup

C3 classification BB

Number of members (P>50%) 70

Radius (P>50% members) 2.6 [arcmin]

C_N 0.6 Moderately populated
C_dens 0.46 Loose
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.57 Likely unique

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

Overview

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CWNU 3215 is a moderately populated, loose object of intermediate C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by very high extinction. It is catalogued as an intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Very distant Very high extinction Intermediate age

Data

🔍 Search references for CWNU 3215 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	–	135.11	-47.986	0.137	-3.277	3.332	58.13
He et al.	2023	135.108	-47.988	0.145	-3.278	3.319	58.13

💡 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	5.62	5.30	–	631	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 2173	42.9	135.11	-47.99	0.14	-3.28	3.34	58.13	0.23

💡 Note: The % column shows the percentage of members that CWNU 3215 shares with each listed object.

Visualization

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