CWNU 3944

0.03 UTI

0.61

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.06

C_dup

C3 classification AA

Number of members (P>50%) 72

Radius (P>50% members) 2.7 [arcmin]

C_N 0.61 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.06 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWNU 3944 is a moderately populated, very dense object of very 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 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.

Distant Very high extinction Very young

Data

🔍 Search references for CWNU 3944 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	–	213.79	-61.859	0.268	-3.968	-2.202	13.048
He et al.	2023	213.783	-61.862	0.274	-3.989	-2.205	13.05

💡 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]	Bfr	BSS
He et al.	2023	4.07	7.40	–	16	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 2642	94.4	213.79	-61.86	0.26	-3.98	-2.2	13.05	0.49

💡 Note: The % column shows the percentage of members that CWNU 3944 shares with each listed object.

Visualization

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