CWWDL 14032

0.05 UTI

0.38

C_N

0.31

C_dens

0.25

C_C3

0.0

C_lit

0.29

C_dup

C3 classification DB

Number of members (P>50%) 38

Radius (P>50% members) 9.0 [arcmin]

C_N 0.38 Poorly populated
C_dens 0.31 Loose
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 0.29 Possibly duplicate

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

Overview

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CWWDL 14032 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a relatively close 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 very 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 14032 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	–	94.499	22.649	0.527	0.425	-1.658	-32.328
Chi et al.	2023	94.48	22.654	0.526	0.415	-1.607	–

💡 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	–	–	–	2	0.120	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1306	71.1	94.62	22.88	0.53	0.45	-1.62	-1.83	0.21
HSC 1502	57.9	94.49	22.64	0.53	0.45	-1.68	–	0.02
FSR 0891	15.8	94.38	22.45	0.54	0.41	-1.71	–	0.19
CWWDL 14038	5.3	94.74	23.16	0.52	0.48	-1.58	-1.83	0.04
OC 0311	2.6	94.37	22.39	0.57	0.47	-1.74	–	0.12

💡 Note: The % column shows the percentage of members that CWWDL 14032 shares with each listed object.

Visualization

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