CWNU 3150

0.01 UTI

0.25

C_N

1.0

C_dens

0.5

C_C3

0.0

C_lit

0.04

C_dup

C3 classification BB

Number of members (P>50%) 25

Radius (P>50% members) 1.6 [arcmin]

C_N 0.25 Poorly populated
C_dens 1.0 Very dense
C_C3 0.5 Intermediate 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 3150 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as an old 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 Moderate extinction Old

Data

🔍 Search references for CWNU 3150 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	–	320.054	44.429	0.226	-4.238	-3.684	-26.724
He et al.	2023	320.053	44.434	0.232	-4.224	-3.694	-26.72

💡 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	3.63	1.30	–	1995	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 694	96.0	320.05	44.43	0.23	-4.24	-3.68	-26.72	0.45

💡 Note: The % column shows the percentage of members that CWNU 3150 shares with each listed object.

Visualization

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