CWWDL 13796

0.10 UTI

0.0

C_N

0.3

C_dens

0.75

C_C3

0.0

C_lit

0.48

C_dup

N₅₀ (P>50% members) 23

Stellar density (N₅₀/rad) 1.5 [N/pc²]

C3 classification AB

C_N 0.0 Sparse
C_dens 0.3 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.48 Possibly duplicate

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWWDL 13796 is a sparse, loose object of high 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 13796 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	99999–	98.969	8.755	0.481	-0.075	-1.326	–
Chi et al.	2023	98.987	8.744	0.471	-0.128	-1.199	–

💡 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]	B_frac	BSS
UCC	99999–	–	–	–	19	-0.280	–	–	–
Chi et al.	2023	–	–	–	19	-0.280	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HXHWL 58	52.0	98.94	8.76	0.48	-0.03	-1.37	–	0.29

💡 Note: The % column shows the percentage of members that CWWDL 13796 shares with each listed object.

Visualization

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