CWWDL 4995

0.01 UTI

0.41

C_N

1.0

C_dens

0.38

C_C3

0.0

C_lit

0.02

C_dup

C3 classification CB

Number of members (P>50%) 41

Radius (P>50% members) 3.0 [arcmin]

C_N 0.41 Poorly populated
C_dens 1.0 Very dense
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.02 Very likely duplicate

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

Overview

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CWWDL 4995 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane. It is catalogued as a near-solar metallicity, 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.

Near-solar metallicity Young

Data

🔍 Search references for CWWDL 4995 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	–	141.315	-52.34	0.407	-5.741	5.401	6.286
Chi et al.	2023	141.317	-52.346	0.41	-5.746	5.349	–

💡 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
Chi et al.	2023	–	–	–	27	0.400	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 1394	97.6	141.3	-52.34	0.39	-5.73	5.41	34.08	0.45

💡 Note: The % column shows the percentage of members that CWWDL 4995 shares with each listed object.

Visualization

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