CWNU 3952

0.02 UTI

0.26

C_N

0.1

C_dens

0.38

C_C3

0.0

C_lit

0.12

C_dup

C3 classification BC

Number of members (P>50%) 26

Radius (P>50% members) 7.5 [arcmin]

C_N 0.26 Poorly populated
C_dens 0.1 Very loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.12 Likely duplicate

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

Overview

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CWNU 3952 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a moderate distance, below 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 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 Young

Data

🔍 Search references for CWNU 3952 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	–	109.498	-19.992	0.306	-1.689	3.345	–
He et al.	2023	109.497	-20.009	0.3	-1.675	3.345	–

💡 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	3.31	1.50	–	79	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1847	88.5	109.5	-20.01	0.32	-1.69	3.35	–	0.09
CWWDL 3813	15.4	109.57	-20.05	0.32	-2.02	3.31	–	0.16

💡 Note: The % column shows the percentage of members that CWNU 3952 shares with each listed object.

Visualization

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