CWNU 3724

0.04 UTI

0.26

C_N

0.18

C_dens

0.75

C_C3

0.0

C_lit

0.15

C_dup

C3 classification AB

Number of members (P>50%) 26

Radius (P>50% members) 4.0 [arcmin]

C_N 0.26 Poorly populated
C_dens 0.18 Very loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.15 Likely duplicate

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

Overview

ℹ️

CWNU 3724 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a moderate distance, near 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 3724 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	117.201	-26.262	0.216	-2.344	3.014	–
He et al.	2023	117.205	-26.273	0.208	-2.349	3.011	–

💡 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	4.57	1.05	–	32	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1945	84.6	117.2	-26.27	0.22	-2.32	3.01	–	0.14

💡 Note: The % column shows the percentage of members that CWNU 3724 shares with each listed object.

Visualization

ℹ️