CWWDL 268

0.09 UTI

0.51

C_N

0.27

C_dens

0.75

C_C3

0.0

C_lit

0.31

C_dup

C3 classification AB

Number of members (P>50%) 52

Radius (P>50% members) 6.8 [arcmin]

C_N 0.51 Moderately populated
C_dens 0.27 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.31 Possibly duplicate

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

Overview

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CWWDL 268 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a moderate distance, below 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 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 Very young

Data

🔍 Search references for CWWDL 268 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	–	109.97	-19.03	0.319	-1.692	1.48	49.45
Chi et al.	2023	109.987	-19.078	0.313	-1.637	1.519	–

💡 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	–	–	–	1	0.440	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 634	69.2	109.94	-18.99	0.32	-1.7	1.42	49.45	0.58
UBC 450	15.4	110.09	-19.37	0.32	-1.85	1.41	93.5	0.46

💡 Note: The % column shows the percentage of members that CWWDL 268 shares with each listed object.

Visualization

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