CWNU 3972

0.14 UTI

0.5

C_N

0.14

C_dens

0.75

C_C3

0.0

C_lit

0.52

C_dup

C3 classification AB

Number of members (P>50%) 50

Radius (P>50% members) 7.6 [arcmin]

C_N 0.5 Moderately populated
C_dens 0.14 Very loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.52 Likely unique

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

Overview

ℹ️

CWNU 3972 is a moderately populated, very loose object of high 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.

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.

Distant Moderate extinction Young

Data

🔍 Search references for CWNU 3972 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	329.519	52.706	0.26	-3.504	-3.681	–
He et al.	2023	329.484	52.7	0.259	-3.489	-3.676	-72.39

💡 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	3.39	1.75	–	25	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 765	48.0	329.38	52.71	0.26	-3.54	-3.66	–	0.17

💡 Note: The % column shows the percentage of members that CWNU 3972 shares with each listed object.

Visualization

ℹ️