CWWDL 14492

0.05 UTI

0.34

C_N

0.29

C_dens

0.75

C_C3

0.0

C_lit

0.18

C_dup

C3 classification AB

Number of members (P>50%) 34

Radius (P>50% members) 14.3 [arcmin]

C_N 0.34 Poorly populated
C_dens 0.29 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.18 Likely duplicate

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

Overview

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CWWDL 14492 is a poorly populated, loose object of high 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 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 14492 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	–	196.141	-57.164	0.862	-6.204	-0.855	-2.312
Chi et al.	2023	196.221	-57.301	0.882	-6.185	-0.846	-3.431

💡 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	–	–	–	4	-0.400	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 27	82.4	196.26	-57.03	0.86	-6.23	-0.84	-2.71	0.24
Theia 1934	38.2	196.38	-56.88	0.85	-6.25	-0.81	-2.71	0.09
OC 0591	23.5	196.33	-56.88	0.85	-6.25	-0.78	-10.22	0.22

💡 Note: The % column shows the percentage of members that CWWDL 14492 shares with each listed object.

Visualization

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