CWNU 1606

0.07 UTI

0.0

C_N

0.16

C_dens

0.75

C_C3

0.0

C_lit

0.36

C_dup

N₅₀ (P>50% members) 22

Stellar density (N₅₀/rad) 0.8 [N/pc²]

C3 classification AB

C_N 0.0 Sparse
C_dens 0.16 Very loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.36 Possibly duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

ℹ️

CWNU 1606 is a sparse, very loose object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by very 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.

Distant Very high extinction Very young

Data

🔍 Search references for CWNU 1606 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	206.223	-62.115	0.286	-6.407	-1.76	21.203
He et al.	2023	206.247	-62.109	0.293	-6.419	-1.757	-53.62

💡 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–	3.02	7.15	–	2	–	–	–	–
He et al.	2023	3.02	7.15	–	2	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Loden 991	64.0	206.22	-62.07	0.3	-6.39	-1.77	21.2	0.37

💡 Note: The % column shows the percentage of members that CWNU 1606 shares with each listed object.

Visualization

ℹ️