CWWDL 14696

0.00 UTI

0.34

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.0

C_dup

C3 classification BA

Number of members (P>50%) 34

Radius (P>50% members) 34.5 [arcmin]

C_N 0.34 Poorly populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

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

Overview

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CWWDL 14696 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a very close distance, above the mid-plane. It is catalogued as a metal-poor, very 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.

Metal-poor Very young

Data

🔍 Search references for CWWDL 14696 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	–	264.35	-7.949	5.11	-11.131	-20.879	-17.797
Chi et al.	2023	264.435	-7.664	5.1	-11.083	-20.904	-17.855

💡 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	–	–	–	1	-0.580	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Mamajek 2	100.0	264.46	-7.93	5.05	-10.85	-20.72	-17.9	0.76
OCSN 216	100.0	264.46	-7.88	5.05	-10.8	-20.7	-17.9	0.04

💡 Note: The % column shows the percentage of members that CWWDL 14696 shares with each listed object.

Visualization

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