CWNU 4035

0.05 UTI

0.34

C_N

0.75

C_dens

0.75

C_C3

0.0

C_lit

0.15

C_dup

N_m (P>50%) 34

Core radius and density 0.9 [pc], 3.8 [pc^-2]

C3 classification BA

C_N 0.34 Poorly populated
C_dens 0.75 Dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.15 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 4035 is a poorly populated, dense 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 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 4035 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–	274.516	-18.975	0.603	0.998	-1.881	35.434
He et al.	2023	274.524	-18.928	0.603	0.99	-1.85	35.43

💡 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–	1.74	3.35	–	10	–	–	–	–
He et al.	2023	1.74	3.35	–	10	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Teutsch 262	85.3	274.52	-18.98	0.6	0.99	-1.88	17.67	0.44

💡 Note: The % column shows the percentage of members that CWNU 4035 shares with each listed object.

Visualization

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