CWNU 3744

0.06 UTI

0.0

C_N

0.63

C_dens

0.62

C_C3

0.0

C_lit

0.24

C_dup

N₅₀ (P>50% members) 17

Stellar density (N₅₀/rad) 3.2 [N/pc²]

C3 classification CA

C_N 0.0 Sparse
C_dens 0.63 Moderately dense
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.24 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 3744 is a sparse, moderately dense object of intermediate 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.

Very distant Moderate extinction Very young

Data

🔍 Search references for CWNU 3744 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–	176.379	-62.431	0.201	-6.536	0.985	–
He et al.	2023	176.374	-62.431	0.206	-6.525	0.987	–

💡 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–	5.25	2.55	–	6	–	–	–	–
He et al.	2023	5.25	2.55	–	6	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Loden 467	76.0	176.38	-62.43	0.21	-6.53	0.99	–	0.46

💡 Note: The % column shows the percentage of members that CWNU 3744 shares with each listed object.

Visualization

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