CWNU 411

0.16 UTI

0.55

C_N

0.48

C_dens

0.38

C_C3

0.0

C_lit

0.58

C_dup

C3 classification CB

Number of members (P>50%) 59

Radius (P>50% members) 8.5 [arcmin]

C_N 0.55 Moderately populated
C_dens 0.48 Loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.58 Likely unique

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

Overview

ℹ️

CWNU 411 is a moderately populated, loose object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is rarely studied 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.

Relatively close Moderate extinction Near-solar metallicity Young

Data

🔍 Search references for CWNU 411 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	306.558	42.638	0.499	-3.062	-4.263	-5.836
He et al.	2022	306.598	42.657	0.51	-3.07	-4.25	–

💡 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.	2022	1.78	2.40	–	32	0.274	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OC 0130	42.4	306.57	42.64	0.5	-3.07	-4.3	–	0.33

💡 Note: The % column shows the percentage of members that CWNU 411 shares with each listed object.

Visualization

ℹ️