CWWDL 13929

0.09 UTI

0.0

C_N

0.61

C_dens

0.75

C_C3

0.0

C_lit

0.32

C_dup

C3 classification AB

Number of members (P>50%) 21

Radius (P>50% members) 4.1 [arcmin]

C_N 0.0 Sparse
C_dens 0.61 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.32 Possibly duplicate

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

Overview

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CWWDL 13929 is a sparse, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, above 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, and a small percentage with at least one entry reported in the same catalogue. See table with shared members information.

Near-solar metallicity Very young

Data

🔍 Search references for CWWDL 13929 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	–	302.826	36.512	0.454	-2.622	-5.788	-28.413
Chi et al.	2023	302.825	36.532	0.476	-2.742	-5.814	-28.413

💡 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	–	–	–	3	-0.280	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 368	68.0	302.86	36.51	0.44	-2.57	-5.78	-42.81	0.54
CWWDL 10272	12.0	302.89	36.57	0.42	-2.78	-5.7	-2.17	0.05
CWWDL 10273	4.0	302.87	36.5	0.43	-2.51	-5.61	–	0.06

💡 Note: The % column shows the percentage of members that CWWDL 13929 shares with each listed object.

Visualization

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