CWWDL 14104

0.04 UTI

0.57

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.08

C_dup

C3 classification AB

Number of members (P>50%) 64

Radius (P>50% members) 8.0 [arcmin]

C_N 0.57 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.08 Very likely duplicate

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

Overview

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CWWDL 14104 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, below 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 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 Very young

Data

🔍 Search references for CWWDL 14104 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	–	173.045	-68.085	0.699	-8.823	0.759	1.537
Chi et al.	2023	173.044	-68.079	0.691	-8.854	0.791	-4.287

💡 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	–	–	–	17	-0.180	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HXHWL 16	92.2	173.13	-68.1	0.69	-8.82	0.75	1.54	0.47
LISC 3316	90.6	173.07	-68.08	0.7	-8.82	0.76	1.54	0.01
Theia 2982	78.1	173.12	-68.1	0.69	-8.82	0.75	1.54	0.02

💡 Note: The % column shows the percentage of members that CWWDL 14104 shares with each listed object.

Visualization

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