CWWDL 13562

0.09 UTI

0.34

C_N

0.51

C_dens

0.25

C_C3

0.0

C_lit

0.41

C_dup

C3 classification CC

Number of members (P>50%) 34

Radius (P>50% members) 5.7 [arcmin]

C_N 0.34 Poorly populated
C_dens 0.51 Moderately dense
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 0.41 Possibly duplicate

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

Overview

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CWWDL 13562 is a poorly populated, moderately dense object of low 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 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 13562 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	–	149.35	-55.542	0.456	-6.405	3.358	12.432
Chi et al.	2023	149.312	-55.546	0.446	-6.301	3.421	28.165

💡 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	–	–	–	8	0.320	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 1843	58.8	149.36	-55.57	0.46	-6.47	3.32	–	0.32

💡 Note: The % column shows the percentage of members that CWWDL 13562 shares with each listed object.

Visualization

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