CWNU 3462

0.06 UTI

0.59

C_N

0.85

C_dens

1.0

C_C3

0.0

C_lit

0.12

C_dup

N₅₀ (P>50% members) 68

Stellar density (N₅₀/rad) 4.2 [N/pc²]

C3 classification AA

C_N 0.59 Moderately populated
C_dens 0.85 Dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.12 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

ℹ️

CWNU 3462 is a moderately populated, dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a very young 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 Very young

Data

🔍 Search references for CWNU 3462 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	207.417	-62.871	0.312	-6.337	-2.018	-24.506
He et al.	2023	207.405	-62.87	0.296	-6.339	-2.018	7.21

💡 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–	3.31	1.8	–	1	–	–	–	–
He et al.	2023	3.31	1.80	–	1	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
G3CC 13	88.2	207.42	-62.87	0.31	-6.33	-2.02	-11.19	0.52
HSC 2612	45.6	207.43	-62.88	0.3	-6.39	-1.98	7.21	0.13

💡 Note: The % column shows the percentage of members that CWNU 3462 shares with each listed object.

Visualization

ℹ️