CWNU 506

0.00 UTI

0.57

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.0

C_dup

N₅₀ (P>50% members) 65

Stellar density (N₅₀/rad) 13.7 [N/pc²]

C3 classification BA

C_N 0.57 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

ℹ️

CWNU 506 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a metal-rich, intermediate-age cluster (see Parameters). It is rarely studied 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, and a significant percentage with at least one entry reported in the same catalogue. See table with shared members information.

Relatively close High extinction Metal-rich Intermediate age

Data

🔍 Search references for CWNU 506 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	277.245	-12.723	0.48	0.637	-1.674	17.92
He et al.	2022	277.246	-12.723	0.52	0.67	-1.68	–

💡 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]	B_frac	BSS
UCC	99999–	2.51	3.12	–	501	0.916	–	–	–
He et al.	2022	2.51	3.12	–	501	0.916	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1020	100.0	277.26	-12.72	0.46	0.62	-1.65	10.83	0.66
CWNU 44	60.0	277.26	-12.72	0.47	0.61	-1.66	18.06	0.0
OC 0032	50.8	277.26	-12.73	0.48	0.62	-1.66	88.27	0.0
HSC 210	10.8	277.31	-12.7	0.57	0.55	-1.62	–	0.06

💡 Note: The % column shows the percentage of members that CWNU 506 shares with each listed object.

Visualization

ℹ️