CWNU 3126

0.02 UTI

0.26

C_N

0.23

C_dens

0.75

C_C3

0.0

C_lit

0.08

C_dup

N_m (P>50%) 26

Core radius and density 0.5 [pc], 1.1 [pc^-2]

C3 classification AB

C_N 0.26 Poorly populated
C_dens 0.23 Very loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.08 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 3126 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a relatively close distance, near 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 very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close High extinction Very young

Data

🔍 Search references for CWNU 3126 in: SciX Simbad

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Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	252.462	-47.293	0.786	0.945	-3.672	-5.279
He et al.	2023	252.44	-47.282	0.792	0.924	-3.672	-55.76

💡 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–	1.29	3.25	–	10	–	–	–	–
He et al.	2023	1.29	3.25	–	10	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 2814	92.3	252.46	-47.29	0.78	0.94	-3.68	-5.28	0.22

💡 Note: The % column shows the percentage of members that CWNU 3126 shares with each listed object.

Visualization

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