CWWDL 14317

0.01 UTI

0.34

C_N

0.38

C_dens

0.5

C_C3

0.0

C_lit

0.03

C_dup

C3 classification BB

Number of members (P>50%) 34

Radius (P>50% members) 13.0 [arcmin]

C_N 0.34 Poorly populated
C_dens 0.38 Loose
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.03 Very likely duplicate

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

Overview

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CWWDL 14317 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is very 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 Young

Data

🔍 Search references for CWWDL 14317 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	–	92.747	6.568	0.897	-0.043	-1.462	-5.574
Chi et al.	2023	92.722	6.77	0.902	-0.056	-1.492	9.978

💡 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	–	–	–	44	0.420	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HXHWL 12	97.1	92.76	6.56	0.89	-0.03	-1.45	9.34	0.47

💡 Note: The % column shows the percentage of members that CWWDL 14317 shares with each listed object.

Visualization

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