CWNU 3346

0.10 UTI

0.61

C_N

0.77

C_dens

0.38

C_C3

0.0

C_lit

0.28

C_dup

C3 classification CB

Number of members (P>50%) 72

Radius (P>50% members) 4.2 [arcmin]

C_N 0.61 Moderately populated
C_dens 0.77 Dense
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.28 Possibly duplicate

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

Overview

ℹ️

CWNU 3346 is a moderately populated, dense object of low C3 quality. Its parallax locates it at a moderate^* distance, above the mid-plane, affected by high extinction. It is catalogued as a very young cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

(*): The parallax distance estimate (~3.54 kpc) differs significantly from the median photometric distance (~5.25 kpc).

Very distant High extinction Very young

Data

🔍 Search references for CWNU 3346 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	99.081	10.902	0.282	-0.593	-1.116	–
He et al.	2023	99.09	10.896	0.263	-0.59	-1.13	–

💡 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	5.25	4.55	–	3	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1598	72.2	99.07	10.91	0.3	-0.6	-1.08	–	0.33

💡 Note: The % column shows the percentage of members that CWNU 3346 shares with each listed object.

Visualization

ℹ️