CWWDL 208

0.33 UTI

0.44

C_N

0.84

C_dens

0.38

C_C3

0.0

C_lit

1.0

C_dup

C3 classification CB

Number of members (P>50%) 44

Radius (P>50% members) 2.5 [arcmin]

C_N 0.44 Poorly populated
C_dens 0.84 Dense
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

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

Overview

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CWWDL 208 is a poorly populated, dense object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a significant percentage of members with 2 later reported entries. See table with shared members information.

Near-solar metallicity Young

Data

🔍 Search references for CWWDL 208 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	–	147.15	-58.67	0.225	-5.241	3.595	22.646
Chi et al.	2023	147.112	-58.664	0.235	-5.315	3.586	11.187

💡 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	–	–	–	93	0.300	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 3358	56.8	147.15	-58.67	0.22	-5.21	3.59	21.47	0.02
HSC 2294	52.3	147.16	-58.67	0.21	-5.2	3.59	21.47	0.09

💡 Note: The % column shows the percentage of members that CWWDL 208 shares with each listed object.

Visualization

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