CWWDL 8488

0.05 UTI

0.0

C_N

0.08

C_dens

0.5

C_C3

0.0

C_lit

0.44

C_dup

C3 classification BB

Number of members (P>50%) 20

Radius (P>50% members) 8.5 [arcmin]

C_N 0.0 Sparse
C_dens 0.08 Very loose
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.44 Possibly duplicate

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

Overview

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CWWDL 8488 is a sparse, very loose object of intermediate 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 possibly a duplicate object, which shares a significant 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 8488 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	–	17.494	62.787	0.349	-2.062	-0.332	-82.232
Chi et al.	2023	17.212	62.841	0.337	-2.05	-0.323	-62.187

💡 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	–	–	–	44	0.400	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OC 0232	56.0	17.63	62.74	0.37	-2.06	-0.34	–	0.31

💡 Note: The % column shows the percentage of members that CWWDL 8488 shares with each listed object.

Visualization

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