CWWDL 3395

0.09 UTI

0.35

C_N

0.53

C_dens

0.5

C_C3

0.0

C_lit

0.34

C_dup

C3 classification BB

Number of members (P>50%) 35

Radius (P>50% members) 3.7 [arcmin]

C_N 0.35 Poorly populated
C_dens 0.53 Moderately dense
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.34 Possibly duplicate

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

Overview

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CWWDL 3395 is a poorly populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane. It is catalogued as a metal-poor, intermediate-age cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Metal-poor Intermediate age

Data

🔍 Search references for CWWDL 3395 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	–	125.633	-45.608	0.297	-3.077	3.846	46.201
Chi et al.	2023	125.653	-45.608	0.315	-3.17	3.909	41.475

💡 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	–	–	–	214	-0.880	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OC 0477	65.7	125.65	-45.62	0.3	-3.05	3.85	46.2	0.3

💡 Note: The % column shows the percentage of members that CWWDL 3395 shares with each listed object.

Visualization

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