CWNU 3414

0.05 UTI

0.34

C_N

0.6

C_dens

0.38

C_C3

0.0

C_lit

0.18

C_dup

C3 classification BC

Number of members (P>50%) 34

Radius (P>50% members) 2.8 [arcmin]

C_N 0.34 Poorly populated
C_dens 0.6 Moderately dense
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.18 Likely duplicate

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

Overview

ℹ️

CWNU 3414 is a poorly populated, moderately dense object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It was recently reported in the literature.

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

Distant Moderate extinction Intermediate age

Data

🔍 Search references for CWNU 3414 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	62.561	47.846	0.243	-0.379	-0.895	-72.036
He et al.	2023	62.565	47.844	0.226	-0.381	-0.892	-72.04

💡 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	3.80	2.95	–	501	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1217	82.4	62.56	47.85	0.24	-0.38	-0.87	-72.04	0.33

💡 Note: The % column shows the percentage of members that CWNU 3414 shares with each listed object.

Visualization

ℹ️