CWWDL 14425

0.00 UTI

0.42

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.0

C_dup

C3 classification AB

Number of members (P>50%) 42

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

C_N 0.42 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 14425 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a close distance, above 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 14425 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	–	195.959	-60.078	1.494	-12.089	-3.865	-2.897
Chi et al.	2023	195.936	-60.07	1.5	-12.021	-3.825	-2.309

💡 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	–	–	–	27	0.440	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 1122	100.0	196.04	-59.99	1.5	-12.07	-3.91	-2.83	0.42
OC 0588	88.1	195.99	-60.09	1.5	-12.09	-3.88	-2.98	0.54
OC 0590	9.5	196.62	-59.91	1.5	-11.98	-4.09	-2.68	0.25

💡 Note: The % column shows the percentage of members that CWWDL 14425 shares with each listed object.

Visualization

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