CWWDL 6302

0.04 UTI

0.5

C_N

0.74

C_dens

0.5

C_C3

0.0

C_lit

0.12

C_dup

C3 classification BB

Number of members (P>50%) 51

Radius (P>50% members) 5.9 [arcmin]

C_N 0.5 Moderately populated
C_dens 0.74 Moderately dense
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.12 Likely duplicate

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

Overview

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CWWDL 6302 is a moderately populated, moderately dense 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, very young cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is 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 Very young

Data

🔍 Search references for CWWDL 6302 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	–	95.913	11.548	0.462	-0.643	-1.161	–
Chi et al.	2023	95.897	11.573	0.474	-0.639	-1.175	–

💡 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	–	–	–	15	0.230	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1319	88.2	95.91	11.53	0.45	-0.64	-1.18	–	0.52

💡 Note: The % column shows the percentage of members that CWWDL 6302 shares with each listed object.

Visualization

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