CWNU 3363

0.22 UTI

0.0

C_N

0.36

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

N_m (P>50%) 23

Core radius and density 1.5 [pc], 1.8 [pc^-2]

C3 classification BA

C_N 0.0 Sparse
C_dens 0.36 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

ℹ️

CWNU 3363 is a sparse, loose object of high C3 quality. Its parallax locates it at a large distance, near the mid-plane, affected by very high extinction. It is catalogued as a young cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Distant Very high extinction Young

Data

🔍 Search references for CWNU 3363 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	282.956	-0.484	0.193	-1.43	-3.513	84.894
He et al.	2023	282.954	-0.485	0.188	-1.422	-3.509	53.02

💡 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–	4.07	5.8	–	63	–	–	–	–
He et al.	2023	4.07	5.80	–	63	–	–	–	–

Visualization

ℹ️